Benjamin J Weiner

Interests

Research

Benjamin Weiner's research investigates the nature and evolution of star-forming and active galaxies from the present day back to half the age of the universe ago. His recent projects grow out of large redshift surveys combined with multi-wavelength data, including far-IR measurements from Spitzer and Herschel, to measure infrared luminosities and star formation rates, and optical spectroscopy to measure redshifts and make detailed analyses of galaxy properties.

Courses

No activities entered.

Scholarly Contributions

Journals/Publications

• Geha, M., Mao, Y., Wechsler, R. H., Asali, Y., Kado-Fong, E., Kallivayalil, N., Nadler, E. O., Tollerud, E. J., Weiner, B., Reyes, M. A., Wang, Y., & Wu, J. F. (2024). The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way\textendashmass Galaxies. \apj, 976(1), 118.
• Kado-Fong, E., Geha, M., Mao, Y., Reyes, M. A., Wechsler, R. H., Asali, Y., Kallivayalil, N., Nadler, E. O., Tollerud, E. J., & Weiner, B. (2024). SAGAbg. I. A Near-unity Mass-loading Factor in Low-mass Galaxies via Their Low-redshift Evolution in Stellar Mass, Oxygen Abundance, and Star Formation Rate. \apj, 966(1), 129.
• Kado-Fong, E., Geha, M., Mao, Y., Reyes, M. A., Wechsler, R. H., Weiner, B., Asali, Y., Kallivayalil, N., Nadler, E. O., Tollerud, E. J., & Wang, Y. (2024). SAGAbg. II. The Low-mass Star-forming Sequence Evolves Significantly between 0.05 < z < 0.21. \apj, 976(1), 83.
• Mao, Y., Geha, M., Wechsler, R. H., Asali, Y., Wang, Y., Kado-Fong, E., Kallivayalil, N., Nadler, E. O., Tollerud, E. J., Weiner, B., Reyes, M. A., & Wu, J. F. (2024). The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way\textendashmass Galaxies. \apj, 976(1), 117.
• Shrestha, M., Pearson, J., Wyatt, S., Sand, D. J., Hosseinzadeh, G., Bostroem, K. A., Andrews, J. E., Dong, Y., Hoang, E., Janzen, D., Jencson, J. E., Lundquist, M., Mehta, D., Retamal, N. M., Valenti, S., Rastinejad, J. C., Daly, P., Porter, D., Hinz, J., , Self, S., et al. (2024). Evidence of Weak Circumstellar Medium Interaction in the Type II SN 2023axu. \apj, 961(2), 247.
• Thornton, J., Amon, A., Wechsler, R. H., Adhikari, S., Mao, Y., Myles, J., Geha, M., Kallivayalil, N., Tollerud, E., & Weiner, B. (2024). The mass profiles of dwarf galaxies from Dark Energy Survey lensing. \mnras, 535(1), 1-20.
• Wang, Y., Nadler, E. O., Mao, Y., Wechsler, R. H., Abel, T., Behroozi, P., Geha, M., Asali, Y., Reyes, M. A., Kado-Fong, E., Kallivayalil, N., Tollerud, E. J., Weiner, B., & Wu, J. F. (2024). The SAGA Survey. V. Modeling Satellite Systems around Milky Way\textendashMass Galaxies with Updated UNIVERSEMACHINE. \apj, 976(1), 119.
• Alexander, D. M., Davis, T. M., Chaussidon, E., Fawcett, V., X., G. A., Lan, T., Y{\`eche}, C., Ahlen, S., Aguilar, J., Armengaud, E., Bailey, S., Brooks, D., Cai, Z., Canning, R., Carr, A., Chabanier, S., Cousinou, M., Dawson, K., Macorra, A., , Dey, A., et al. (2023). The DESI Survey Validation: Results from Visual Inspection of the Quasar Survey Spectra. \aj, 165(3), 124.
• Arrabal, H. P., Dickinson, M., Finkelstein, S. L., Fujimoto, S., Fern{\'andez}, V., Kartaltepe, J. S., Jung, I., Cole, J. W., Burgarella, D., Chworowsky, K., Hutchison, T. A., Morales, A. M., Papovich, C., Simons, R. C., Amor{\'\in}, R. O., Backhaus, B. E., Bagley, M. B., Bisigello, L., Calabr{\`o}, A., , Castellano, M., et al. (2023). Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z ??? 8-10. \apjl, 951(1), L22.
• Arrabal, H. P., Dickinson, M., Finkelstein, S. L., Kartaltepe, J. S., Donnan, C. T., Burgarella, D., Carnall, A. C., Cullen, F., Dunlop, J. S., Fern{\'andez}, V., Fujimoto, S., Jung, I., Krips, M., Larson, R. L., Papovich, C., P{\'erez-Gonz\'alez}, P. G., Amor{\'\in}, R. O., Bagley, M. B., Buat, V., , Casey, C. M., et al. (2023). Confirmation and refutation of very luminous galaxies in the early Universe. \nat, 622(7984), 707-711.
• Chen, Y., Jones, T., Sanders, R., Fadda, D., Sutter, J., Minchin, R., Huntzinger, E., Senchyna, P., Stark, D., Spilker, J., Weiner, B., & Roberts-Borsani, G. (2023). Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra. Nature Astronomy, 7, 771-778.
• Cleri, N. J., Yang, G., Papovich, C., Trump, J. R., Backhaus, B. E., Estrada-Carpenter, V., Finkelstein, S. L., Giavalisco, M., Hutchison, T. A., Ji, Z., Jung, I., Matharu, J., Momcheva, I., Olivier, G. M., Simons, R., & Weiner, B. (2023). CLEAR: High-ionization [Ne V] \ensuremath{\lambda}3426 Emission-line Galaxies at 1.4 < z < 2.3. \apj, 948(2), 112.
• Darragh-Ford, E., Wu, J. F., Mao, Y., Wechsler, R. H., Geha, M., Forero-Romero, J. E., Hahn, C., Kallivayalil, N., Moustakas, J., Nadler, E. O., Nowotka, M., Peek, J., Tollerud, E. J., Weiner, B., Aguilar, J., Ahlen, S., Brooks, D., Cooper, A., Macorra, A., , Dey, A., et al. (2023). Target Selection and Sample Characterization for the DESI LOW-Z Secondary Target Program. \apj, 954(2), 149.
• Estrada-Carpenter, V., Papovich, C., Momcheva, I., Brammer, G., Simons, R. C., Cleri, N. J., Giavalisco, M., Matharu, J., Trump, J. R., Weiner, B., & Ji, Z. (2023). CLEAR: The Morphological Evolution of Galaxies in the Green Valley. \apj, 951(2), 115.
• Finkelstein, S. L., Bagley, M. B., Ferguson, H. C., Wilkins, S. M., Kartaltepe, J. S., Papovich, C., Yung, L. A., Arrabal, H. P., Behroozi, P., Dickinson, M., Kocevski, D. D., Koekemoer, A. M., Larson, R. L., Le, B. A., Morales, A. M., P{\'erez-Gonz\'alez}, P. G., Burgarella, D., Dav{\'e}, R., Hirschmann, M., , Somerville, R. S., et al. (2023). CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST. \apjl, 946(1), L13.
• Fujimoto, S., Finkelstein, S. L., Burgarella, D., Carilli, C. L., Buat, V., Casey, C. M., Ciesla, L., Tacchella, S., Zavala, J. A., Brammer, G., Fudamoto, Y., Ouchi, M., Valentino, F., Cooper, M., Dickinson, M., Franco, M., Giavalisco, M., Hutchison, T. A., Kartaltepe, J. S., , Koekemoer, A. M., et al. (2023). ALMA FIR View of Ultra-high-redshift Galaxy Candidates at z \ensuremath{\sim} 11-17: Blue Monsters or Low-z Red Interlopers?. \apj, 955(2), 130.
• Hahn, C., Kwon, K., Tojeiro, R., Siudek, M., Canning, R. E., Mezcua, M., Tinker, J. L., Brooks, D., Doel, P., Fanning, K., Gazta{\~naga}, E., Kehoe, R., Landriau, M., Meisner, A., Moustakas, J., Poppett, C., Tarle, G., Weiner, B., & Zou, H. u. (2023). The DESI PRObabilistic Value-added Bright Galaxy Survey (PROVABGS) Mock Challenge. \apj, 945(1), 16.
• Lan, T., Tojeiro, R., Armengaud, E., Prochaska, J. X., Davis, T., Alexander, D. M., Raichoor, A., Zhou, R., Y{\`eche}, C., Balland, C., BenZvi, S., Berti, A., Canning, R., Carr, A., Chittenden, H., Cole, S., Cousinou, M. -., Dawson, K., Dey, B., , Douglass, K., et al. (2023). The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies. \apj, 943(1), 68.
• Larson}, R. L., Finkelstein, S. L., Kocevski, D. D., Hutchison, T. A., Trump, J. R., Arrabal, H. P., Bromm, V., Cleri, N. J., Dickinson, M., Fujimoto, S., Kartaltepe, J. S., Koekemoer, A. M., Papovich, C., Pirzkal, N., Tacchella, S., Zavala, J. A., Bagley, M., Behroozi, P., Champagne, J. B., , Cole, J. W., et al. (2023). A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars. \apjl, 953(2), L29.
• Napolitano, L., Pandey, A., Myers, A. D., Lan, T., Anand, A., Aguilar, J., Ahlen, S., Alexander, D. M., Brooks, D., Canning, R., Circosta, C., De, L., Doel, P., Eftekharzadeh, S., Fawcett, V. A., Font-Ribera, A., Garcia-Bellido, J., Gontcho, A., Le Guillou, L., , Guy, J., et al. (2023). Detecting and Characterizing Mg II Absorption in DESI Survey Validation Quasar Spectra. \aj, 166(3), 99.
• Papovich, C., Cole, J. W., Yang, G., Finkelstein, S. L., Barro, G., Buat, V., Burgarella, D., P{\'erez-Gonz\'alez}, P. G., Santini, P., Seill{\'e}, L., Shen, L. u., Arrabal, H. P., Bagley, M. B., Bell, E. F., Bisigello, L., Calabr{\`o}, A., Casey, C. M., Castellano, M., Chworowsky, K., , Cleri, N. J., et al. (2023). CEERS Key Paper. V. Galaxies at 4 < z < 9 Are Bluer than They Appear\textendashCharacterizing Galaxy Stellar Populations from Rest-frame \ensuremath{\sim}1 \ensuremath{\mu}m Imaging. \apjl, 949(2), L18.
• Shen, L. u., Papovich, C., Yang, G., Matharu, J., Wang, X., Magnelli, B., Elbaz, D., Jogee, S., Alavi, A., Arrabal, H. P., Backhaus, B. E., Bagley, M. B., Bell, E. F., Bisigello, L., Calabr{\`o}, A., Cooper, M., Costantin, L., Daddi, E., Dickinson, M., , Finkelstein, S. L., et al. (2023). CEERS: Spatially Resolved UV and Mid-infrared Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes. \apj, 950(1), 7.
• Simons, R. C., Papovich, C., Momcheva, I. G., Brammer, G., Estrada-Carpenter, V., Finkelstein, S. L., Gosmeyer, C. M., Matharu, J., Trump, J. R., Backhaus, B. E., Cheng, Y., Cleri, N. J., Ferguson, H. C., Finlator, K., Giavalisco, M., Ji, Z., Jung, I., Lotz, J. M., O'Brien, R., , Skelton, R. E., et al. (2023). CLEAR: Survey Overview, Data Analysis, and Products. \apjs, 266(1), 13.
• Trump, J. R., Arrabal, H. P., Simons, R. C., Backhaus, B. E., Amor{\'\in}, R. O., Dickinson, M., Fern{\'andez}, V., Papovich, C., Nicholls, D. C., Kewley, L. J., Brunker, S. W., Salzer, J. J., Wilkins, S. M., Almaini, O., Bagley, M. B., Berg, D. A., Bhatawdekar, R., Bisigello, L., Buat, V., , Burgarella, D., et al. (2023). The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations. \apj, 945(1), 35.
• Zavala}, J. A., Buat, V., Casey, C. M., Finkelstein, S. L., Burgarella, D., Bagley, M. B., Ciesla, L., Daddi, E., Dickinson, M., Ferguson, H. C., Franco, M., Jim{\'enez-Andrade}, E., Kartaltepe, J. S., Koekemoer, A. M., Le, B. A., Murphy, E., Papovich, C., Tacchella, S., Wilkins, S. M., , Aretxaga, I., et al. (2023). Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations. \apjl, 943(2), L9.
• Backhaus, B. E., Trump, J. R., Cleri, N. J., Simons, R., Momcheva, I., Papovich, C., Estrada-Carpenter, V., Finkelstein, S. L., Matharu, J., Ji, Z., Weiner, B., Giavalisco, M., & Jung, I. (2022). CLEAR: Emission-line Ratios at Cosmic High Noon. \apj, 926(2), 161.
• Cleri, N. J., Trump, J. R., Backhaus, B. E., Momcheva, I., Papovich, C., Simons, R., Weiner, B., Estrada-Carpenter, V., Finkelstein, S. L., Giavalisco, M., Ji, Z., Jung, I., Matharu, J., Martinez, F., & Sturm, M. R. (2022). CLEAR: Paschen-\ensuremath{\beta} Star Formation Rates and Dust Attenuation of Low-redshift Galaxies. \apj, 929(1), 3.
• Cooper, J. R., Rudnick, G. H., Brammer, G. G., Desjardins, T., Mann, J. L., Weiner, B. J., Arag{\'on-Salamanca}, A., De, L. G., Desai, V., Finn, R. A., Jablonka, P., Jaff{\'e}, Y. L., Moustakas, J., Sp{\'erone-Longin}, D., Teplitz, H. I., Vulcani, B., & Zaritsky, D. (2022). H \ensuremath{\alpha}-based star formation rates in and around z 0.5 EDisCS clusters. \mnras, 509(4), 5382-5398.
• Finkelstein}, S. L., Bagley, M. B., Arrabal, H. P., Dickinson, M., Ferguson, H. C., Kartaltepe, J. S., Papovich, C., Burgarella, D., Kocevski, D. D., Huertas-Company, M., Iyer, K. G., Koekemoer, A. M., Larson, R. L., P{\'erez-Gonz\'alez}, P. G., Rose, C., Tacchella, S., Wilkins, S. M., Chworowsky, K., Medrano, A., , Morales, A. M., et al. (2022). A Long Time Ago in a Galaxy Far, Far Away: A Candidate z \ensuremath{\sim} 12 Galaxy in Early JWST CEERS Imaging. \apjl, 940(2), L55.
• Matharu, J., Papovich, C., Simons, R. C., Momcheva, I., Brammer, G., Ji, Z., Backhaus, B. E., Cleri, N. J., Estrada-Carpenter, V., Finkelstein, S. L., Finlator, K., Giavalisco, M., Jung, I., Muzzin, A., Nelson, E. J., Pillepich, A., Trump, J. R., & Weiner, B. (2022). CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between 0.5 \ensuremath{\lesssim} z \ensuremath{\lesssim} 1.7 Using H\ensuremath{\alpha} Emission Line Maps. \apj, 937(1), 16.
• Papovich, C., Simons, R. C., Estrada-Carpenter, V., Matharu, J., Momcheva, I., Trump, J. R., Backhaus, B. E., Brammer, G., Cleri, N. J., Finkelstein, S. L., Giavalisco, M., Ji, Z., Jung, I., Kewley, L. J., Nicholls, D. C., Pirzkal, N., Rafelski, M., & Weiner, B. (2022). CLEAR: The Ionization and Chemical-enrichment Properties of Galaxies at 1.1 < z < 2.3. \apj, 937(1), 22.
• Wang, W., Kassin, S. A., Faber, S., Koo, D. C., Cunningham, E. C., Yesuf, H. M., Barro, G., Guhathakurta, P., Weiner, B. J., Vega, A., Guo, Y., Heckman, T. M., Pacifici, C., Wang, B., & Welker, C. (2022). The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-forming Galaxy at z = 1.3. \apj, 930(2), 146.
• Wu, J. F., Peek, J., Tollerud, E. J., Mao, Y., Nadler, E. O., Geha, M., Wechsler, R. H., Kallivayalil, N., & Weiner, B. J. (2022). Extending the SAGA Survey (xSAGA). I. Satellite Radial Profiles as a Function of Host-galaxy Properties. \apj, 927(1), 121.
• Alberts, S., Lee, K., Pope, A., Brodwin, M., Chiang, Y., McKinney, J., Xue, R., Huang, Y., Brown, M., Dey, A., Eisenhardt, P. R., Jannuzi, B. T., Popescu, R., Ramakrishnan, V., Stanford, S. A., & Weiner, B. J. (2021). Measuring the total infrared light from galaxy clusters at z = 0.5-1.6: connecting stellar populations to dusty star formation. \mnras, 501(2), 1970-1998.
• Mao, Y., Geha, M., Wechsler, R. H., Weiner, B., Tollerud, E. J., Nadler, E. O., & Kallivayalil, N. (2021). The SAGA Survey. II. Building a Statistical Sample of Satellite Systems around Milky Way-like Galaxies. \apj, 907(2), 85.
• Paterson, K., Lundquist, M., Rastinejad, J., Fong, W., Sand, D., Andrews, J., Amaro, R., Eskandari, O., Wyatt, S., Daly, P., Bradley, H., Zhou-Wright, S. .., Valenti, S., Yang, S., Christensen, E., Gibbs, A., Shelly, F., Bilinski, C., Chomiuk, L., , Corsi, A., et al. (2021). Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run. \apj, 912(2), 128.
• Simons, R. C., Papovich, C., Momcheva, I., Trump, J. R., Brammer, G., Estrada-Carpenter, V., Backhaus, B. E., Cleri, N. J., Finkelstein, S. L., Giavalisco, M., Ji, Z., Jung, I., Matharu, J., & Weiner, B. (2021). CLEAR: The Gas-phase Metallicity Gradients of Star-forming Galaxies at 0.6 < z < 2.6. \apj, 923(2), 203.
• Williams, C. C., Spilker, J. S., Whitaker, K. E., Dav{\'e}, R., Woodrum, C., Brammer, G., Bezanson, R., Narayanan, D., & Weiner, B. (2021). ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z \ensuremath{\sim} 1.5. \apj, 908(1), 54.
• Chen, H., Zahedy, F. S., Boettcher, E., Cooper, T. M., Johnson, S. D., Rudie, G. C., Chen, M. C., Walth, G. L., Cantalupo, S., Cooksey, K. L., Faucher-Gigu{\`ere}, C., Greene, J. E., Lopez, S., Mulchaey, J. S., Penton, S. V., Petitjean, P., Putman, M. E., Rafelski, M., Rauch, M., , Schaye, J., et al. (2020). The Cosmic Ultraviolet Baryon Survey (CUBS) - I. Overview and the diverse environments of Lyman limit systems at z < 1. \mnras, 497(1), 498-520.
• Estrada-Carpenter, V., Papovich, C., Momcheva, I., Brammer, G., Simons, R., Bridge, J., Cleri, N. J., Ferguson, H., Finkelstein, S. L., Giavalisco, M., Jung, I., Matharu, J., Trump, J. R., & Weiner, B. (2020). CLEAR. II. Evidence for Early Formation of the Most Compact Quiescent Galaxies at High Redshift. \apj, 898(2), 171.
• Weiner, B., Pearce, E., Krantz, H., Block, A., Howie, R., Kattner, S., Self, S., & Williams, G. (2020). MMT/Binospec spectroscopy of near earth object 2020 SO distinguishes it from common natural asteroids. The Astronomer's Telegram, 14241, 1.
• Bezanson, R., Spilker, J., Williams, C. C., Whitaker, K. E., Narayanan, D., Weiner, B., & Franx, M. (2019). Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z=1.522.
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  One of the greatest challenges to theoretical models of massive galaxyformation is the regulation of star formation at early times. The relativeroles of molecular gas expulsion, depletion, and stabilization are uncertain asdirect observational constraints of the gas reservoirs in quenched or quenchinggalaxies at high redshift are scant. We present ALMA observations of CO(2-1) ina massive ($\log M_{\star}/M_{\odot}=11.2$), recently quenched galaxy at$z=1.522$. The optical spectrum of this object shows strong Balmer absorptionlines, which implies that star formation ceased $\sim$0.8 Gyr ago. We do notdetect CO(2-1) line emission, placing an upper limit on the molecular$\mathrm{H_2}$ gas mass of 1.1$\times10^{10}\,M_{\odot}$. The implied gasfraction is $f_{\rm{H_2}}{\equiv M_{H_2}/M_{\star}}1$ passivegalaxy to date. Our observations show that the depletion of $\mathrm{H_2}$ fromthe interstellar medium of quenched objects can be both efficient and fairlycomplete, in contrast to recent claims of significant cold gas in recentlyquenched galaxies. We explore the variation in observed gas fractions inhigh-$z$ galaxies and show that galaxies with high stellar surface density havelow $f_{\rm{H_2}}$, similar to recent correlations between specific starformation rate and stellar surface density.[Journal_ref: ]
• Bezanson, R., Spilker, J., Williams, C. C., Whitaker, K. E., Narayanan, D., Weiner, B., & Franx, M. (2019). Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z = 1.522. \apjl, 873(2), L19.
• Estrada-Carpenter, V., Papovich, C., Momcheva, I., Brammer, G., Long, J., Quadri, R. F., Bridge, J., Dickinson, M., Ferguson, H., Finkelstein, S., Giavalisco, M., Gosmeyer, C. M., Lotz, J., Salmon, B., Skelton, R. E., Trump, J. R., & Weiner, B. (2019). CLEAR. I. Ages and Metallicities of Quiescent Galaxies at 1.0 \< z \< 1.8 Derived from Deep Hubble Space Telescope Grism Data. \apj, 870(2), 133.
• Freundlich, J., Combes, F., Tacconi, L., Genzel, R., Garcia-Burillo, S. .., Neri, R., Contini, T., Bolatto, A., Lilly, S., Salom{\'e}, P., Bicalho, I., Boissier, J., Boone, F., Bouch{\'e}, N., Bournaud, F., Burkert, A., Carollo, M., Cooper, M., Cox, P., , Feruglio, C., et al. (2019). PHIBSS2: survey design and z = 0.5 - 0.8 results. Molecular gas reservoirs during the winding-down of star formation. \aap, 622, A105.
• Lundquist, M., Paterson, K., Fong, W., Sand, D., Andrews, J., Shivaei, I., Daly, P., Valenti, S., Yang, S., Christensen, E., Gibbs, A., Shelly, F., Wyatt, S., Eskandari, O., Kuhn, O., Amaro, R., Arcavi, I., Behroozi, P., Butler, N., , Chomiuk, L., et al. (2019). Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo\textquoterights Third Observing Run. \apjl, 881(2), L26.
• Spilker, J. S., Bezanson, R., Weiner, B. J., Whitaker, K. E., & Williams, C. C. (2019). Evidence for Inside-out Galaxy Growth and Quenching of a z ̃ 2 Compact Galaxy From High-resolution Molecular Gas Imaging. \apj, 883(1), 81.
• Walth, G. L., Egami, E., Cl{\'ement}, B., Rawle, T. D., Rex, M., Richard, J., P{\'erez-Gonz\'alez}, P., Boone, F., Dessauges-Zavadsky, M., Portouw, J., Weiner, B., McGreer, I., & Schneider, E. (2019). Infrared Galaxies in the Field of the Massive Cluster Abell S1063: Discovery of a Luminous Kiloparsec-sized H II Region in a Gravitationally Lensed Infrared-luminous Galaxy at z = 0.6. \apj, 877(1), 7.
• Williams, C. C., Labbe, I., Spilker, J., Stefanon, M., Leja, J., Whitaker, K., Bezanson, R., Narayanan, D., Oesch, P., & Weiner, B. (2019). Discovery of a Dark, Massive, ALMA-only Galaxy at z ̃ 5-6 in a Tiny 3 mm Survey. \apj, 884(2), 154.
• Zahedy}, F. S., Chen, H., Johnson, S. D., Pierce, R. M., Rauch, M., Huang, Y., Weiner, B. J., & Gauthier, J. (2019). Characterizing circumgalactic gas around massive ellipticals at z \ensuremath{\sim} 0.4 - II. Physical properties and elemental abundances. \mnras, 484(2), 2257-2280.
• Zhou, R., Cooper, M. C., Newman, J. A., Ashby, M. L., Aird, J., Conselice, C. J., Davis, M., Dutton, A. A., Faber, S., Fang, J. J., Fazio, G., Guhathakurta, P., Kocevski, D., Koo, D. C., {Nand, r. K., Phillips, A. C., Rosario, D. J., Schlafly, E. F., Trump, J. R., , Weiner, B., et al. (2019). Deep ugrizY imaging and DEEP2/3 spectroscopy: a photometric redshift testbed for LSST and public release of data from the DEEP3 Galaxy Redshift Survey. \mnras, 488(4), 4565-4584.
• Ashcraft, T. A., Windhorst, R. A., Jansen, R. A., Cohen, S. H., Grazian, A., Paris, D., Fontana, A., Giallongo, E., Speziali, R., Testa, V., Boutsia, K., O'Connell, R. W., Rutkowski, M. J., Ryan, R. E., Scarlata, C., & Weiner, B. (2018). Ultra-deep Large Binocular Camera U-band Imaging of the GOODS-North Field: Depth Versus Resolution. Publications of the Astronomical Society of the Pacific, 130(988), 064102.
• Bera, A., Kanekar, N., Weiner, B. J., Sethi, S., & Dwarakanath, K. (2018). Probing Star Formation in Galaxies at z \ensuremath{\approx} 1 via a Giant Metrewave Radio Telescope Stacking Analysis. \apj, 865(1), 39.
• Blanchard, P., Gomez, S., Berger, E., Nicholl, M., Kattner, S., & Weiner, B. (2018). Classification of AT2018bym as a Type I Superluminous Supernova. The Astronomer's Telegram, 11714, 1.
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• Spilker, J., Bezanson, R., Bari{\v{s}i\'c}, I., Bell, E., Lagos, C., Maseda, M., Muzzin, A., Pacifici, C., Sobral, D., Straatman, C., Wel, A., Dokkum, P., Weiner, B., Whitaker, K., Williams, C. C., & Wu, P. (2018). Molecular Gas Contents and Scaling Relations for Massive, Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey. \apj, 860(2), 103.
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• Simons, R., Kassin, S., Weiner, B., Faber, S., Trump, J., Heckman, T., Koo, D., Pacifici, C., Primack, J., Snyder, G., & Vega, A. (2017). z \tilde 2: An Epoch of Disk Assembly. \apj, 843, 46.
• Tinker, J., Brownstein, J., Guo, H., Leauthaud, A., Maraston, C., Masters, K., Montero-Dorta, A., Thomas, D., Tojeiro, R., Weiner, B., Zehavi, I., & Olmstead, M. (2017). The Correlation between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe. \apj, 839, 121.
• Bezanson, R., Wake, D. A., Brammer, G. B., van, D., Franx, M., Labbe, I., Leja, J., Momcheva, I. G., Nelson, E. J., Quadri, R. F., Skelton, R. E., Weiner, B. J., & Whitaker, K. E. (2016). LEVERAGING 3D-HST GRISM REDSHIFTS TO QUANTIFY PHOTOMETRIC REDSHIFT PERFORMANCE. ASTROPHYSICAL JOURNAL, 822(1).
• Huang, Y., Chen, H., Johnson, S. D., & Weiner, B. J. (2016). Characterizing the chemically enriched circumgalactic medium of similar to 38 000 luminous red galaxies in SDSS DR12. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 455(2), 1713-1727.
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• Pacifici, C., Kassin, S. A., Weiner, B. J., Holden, B., Gardner, J. P., Faber, S. M., Ferguson, H. C., Koo, D. C., Primack, J. R., Bell, E. F., Dekel, A., Gawiser, E., Giavalisco, M., Rafelski, M., Simons, R. C., Barro, G., Croton, D. J., Dave, R., Fontana, A., , Grogin, N. A., et al. (2016). THE EVOLUTION OF STAR FORMATION HISTORIES OF QUIESCENT GALAXIES. ASTROPHYSICAL JOURNAL, 832(1).
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• {Kelly}, P., {Brammer}, G., {Selsing}, J., {Foley}, R., {Hjorth}, J., {Rodney}, S., {Christensen}, L., {Strolger}, L., {Filippenko}, A., {Treu}, T., {Steidel}, C., {Strom}, A., {Riess}, A., {Zitrin}, A., {Schmidt}, K., {Brada{\v c}}, M., {Jha}, S., {Graham}, M., {McCully}, C., , {Graur}, O., et al. (2016). SN Refsdal: Classification as a Luminous and Blue SN 1987A-like Type II Supernova. \apj, 831, 205.
• {Kelly}, P., {Rodney}, S., {Treu}, T., {Strolger}, L., {Foley}, R., {Jha}, S., {Selsing}, J., {Brammer}, G., {Brada{\v c}}, M., {Cenko}, S., {Graur}, O., {Filippenko}, A., {Hjorth}, J., {McCully}, C., {Molino}, A., {Nonino}, M., {Riess}, A., {Schmidt}, K., {Tucker}, B., , Linden}, A., et al. (2016). Deja Vu All Over Again: The Reappearance of Supernova Refsdal. \apjl, 819, L8.
• {Rawle}, T., {Altieri}, B., {Egami}, E., {P{\'e}rez-Gonz{\'a}lez}, P., {Boone}, F., {Clement}, B., {Ivison}, R., {Richard}, J., {Rujopakarn}, W., {Valtchanov}, I., {Walth}, G., {Weiner}, B., {Blain}, A., {Dessauges-Zavadsky}, M., {Kneib}, J., {Lutz}, D., {Rodighiero}, G., {Schaerer}, D., , I. (2016). A complete census of Herschel-detected infrared sources within the HST Frontier Fields. \mnras, 459, 1626-1645.
• {Rodney}, S., {Strolger}, L., {Kelly}, P., {Brada{\v c}}, M., {Brammer}, G., {Filippenko}, A., {Foley}, R., {Graur}, O., {Hjorth}, J., {Jha}, S., {McCully}, C., {Molino}, A., {Riess}, A., {Schmidt}, K., {Selsing}, J., {Sharon}, K., {Treu}, T., {Weiner}, B., , A. (2016). SN Refsdal: Photometry and Time Delay Measurements of the First Einstein Cross Supernova. \apj, 820, 50.
• {Rujopakarn}, W., {Dunlop}, J., {Rieke}, G., {Ivison}, R., {Cibinel}, A., {Nyland}, K., {Jagannathan}, P., {Silverman}, J., {Alexander}, D., {Biggs}, A., {Bhatnagar}, S., {Ballantyne}, D., {Dickinson}, M., {Elbaz}, D., {Geach}, J., {Hayward}, C., {Kirkpatrick}, A., {McLure}, R., {Micha{\l}owski}, M., , {Miller}, N., et al. (2016). VLA and ALMA Imaging of Intense Galaxy-wide Star Formation in z {\tilde} 2 Galaxies. \apj, 833, 12.
• {Simons}, R., {Kassin}, S., {Trump}, J., {Weiner}, B., {Heckman}, T., {Barro}, G., {Koo}, D., {Guo}, Y., {Pacifici}, C., {Koekemoer}, A., , A. (2016). Kinematic Downsizing at z {\tilde} 2. \apj, 830, 14.
• Alam, S., Albareti, F. D., Allende, P. C., Anders, F., Anderson, S. F., Anderton, T., Andrews, B. H., Armengaud, E., Aubourg, E., Bailey, S., Basu, S., Bautista, J. E., Beaton, R. L., Beers, T. C., Bender, C. F., Berlind, A. A., Beutler, F., Bhardwaj, V., Bird, J. C., , Bizyaev, D., et al. (2015). THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 219(1).
• Genzel, R., Tacconi, L. J., Lutz, D., Saintonge, A., Berta, S., Magnelli, B., Combes, F., Garcia-Burillo, S., Neri, R., Bolatto, A., Contini, T., Lilly, S., Boissier, J., Boone, F., Bouche, N., Bournaud, F., Burkert, A., Carollo, M., Colina, L., , Cooper, M. C., et al. (2015). COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS. ASTROPHYSICAL JOURNAL, 800(1).
• Kartaltepe, J. S., Mozena, M., Kocevski, D., McIntosh, D. H., Lotz, J., Bell, E. F., Faber, S., Ferguson, H., Koo, D., Bassett, R., Bernyk, M., Blancato, K., Bournaud, F., Cassata, P., Castellano, M., Cheung, E., Conselice, C. J., Croton, D., Dahlen, T., , De, M., et al. (2015). CANDELS VISUAL CLASSIFICATIONS: SCHEME, DATA RELEASE, AND FIRST RESULTS. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 221(1).
• Kelly, P. L., Rodney, S. A., Treu, T., Foley, R. J., Brammer, G., Schmidt, K. B., Zitrin, A., Sonnenfeld, A., Strolger, L., Graur, O. r., Filippenko, A. V., Jha, S. W., Riess, A. G., Bradac, M., Weiner, B. J., Scolnic, D., Malkan, M. A., von, d., Trenti, M., , Hjorth, J., et al. (2015). Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens. SCIENCE, 347(6226), 1123-1126.
• Mei, S., Scarlata, C., Pentericci, L., Newman, J. A., Weiner, B. J., Ashby, M., Castellano, M., Conselice, C. J., Finkelstein, S. L., Galametz, A., Grogin, N. A., Koekemoer, A. M., Huertas-Company, M., Lani, C., Lucas, R. A., Papovich, C., Rafelski, M., & Teplitz, H. I. (2015). STAR-FORMING BLUE ETGS IN TWO NEWLY DISCOVERED GALAXY OVERDENSITIES IN THE HUDF AT z=1.84 AND 1.9: UNVEILING THE PROGENITORS OF PASSIVE ETGS IN CLUSTER CORES. ASTROPHYSICAL JOURNAL, 804(2).
• Morris, A. M., Kocevski, D. D., Trump, J. R., Weiner, B. J., Hathi, N. P., Barro, G., Dahlen, T., Faber, S. M., Finkelstein, S. L., Fontana, A., Ferguson, H. C., Grogin, N. A., Gruetzbauch, R., Guo, Y., Hsu, L., Koekemoer, A. M., Koo, D. C., Mobasher, B., Pforr, J., , Salvato, M., et al. (2015). A WFC3 GRISM EMISSION LINE REDSHIFT CATALOG IN THE GOODS-SOUTH FIELD. ASTRONOMICAL JOURNAL, 149(6).
• Penner, K., Dickinson, M., Weiner, B., Inami, H., Kartaltepe, J., Pforr, J., Nayyeri, H., Kassin, S., Papovich, C., & Pope, A. (2015). Dusty galaxies and the degeneracy between their dust distributions and the attenuation formula.
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  Do spatial distributions of dust grains in galaxies have typical forms, as dospatial distributions of stars? We investigate whether or not the distributionsresemble uniform foreground screens, as commonly assumed by the high-redshiftgalaxy community. We use rest-frame infrared, ultraviolet, and H$\alpha$ lineluminosities of dust-poor and dusty galaxies at z ~ 0 and z ~ 1 to comparemeasured H$\alpha$ escape fractions with those predicted by the Calzettiattenuation formula. The predictions, based on UV escape fractions,overestimate the measured H$\alpha$ escape fractions for all samples. Theinterpretation of this result for dust-poor z ~ 0 galaxies is that regions withionizing stars have more dust than regions with nonionizing UV-emitting stars.Dust distributions for these galaxies are nonuniform. The interpretation of theoverestimates for dusty galaxies at both redshifts is less clear. If theattenuation formula is inapplicable to these galaxies, perhaps thedisagreements are unphysical; perhaps dust distributions in these galaxies areuniform. If the attenuation formula does apply, then dusty galaxies havenonuniform dust distributions; the distributions are more uniform than they arein dust-poor galaxies. A broad range of H$\alpha$ escape fractions at a givenUV escape fraction for z ~ 1 dusty galaxies, if real, indicates diverse dustmorphologies and the implausibility of the screen assumption.[Journal_ref: ]
• Simons, R. C., Kassin, S. A., Weiner, B. J., Heckman, T. M., Lee, J. C., Lotz, J. M., Peth, M., & Tchernyshyov, K. (2015). A transition mass in the local Tully-Fisher relation. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 452(1), 986-997.
• Williams, C. C., Giavalisco, M., Lee, B., Tundo, E., Mobasher, B., Nayyeri, H., Ferguson, H. C., Koekemoer, A., Trump, J. R., Cassata, P., Dekel, A., Guo, Y., Lee, K., Pentericci, L., Bell, E. F., Castellano, M., Finkelstein, S. L., Fontana, A., Grazian, A., , Grogin, N., et al. (2015). THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z similar to 2. ASTROPHYSICAL JOURNAL, 800(1).
• {Alam}, S., {Albareti}, F., {Allende Prieto}, C., {Anders}, F., {Anderson}, S., {Anderton}, T., {Andrews}, B., {Armengaud}, E., {Aubourg}, {., {Bailey}, S., & al., e. (2015). "{The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III}". apjs, 219, 12.
• {Genzel}, R., {Tacconi}, L., {Lutz}, D., {Saintonge}, A., {Berta}, S., {Magnelli}, B., {Combes}, F., {Garc{'{i}}a-Burillo}, S., {Neri}, R., {Bolatto}, A., {Contini}, T., {Lilly}, S., {Boissier}, J., {Boone}, F., {Bouch{'e}}, N., {Bournaud}, F., {Burkert}, A., {Carollo}, M., {Colina}, L., , {Cooper}, M., et al. (2015). "{Combined CO and Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star-formation Rate, and Stellar Mass}". apj, 800, 20.
• {Kartaltepe}, J., {Mozena}, M., {Kocevski}, D., {McIntosh}, D., {Lotz}, J., {Bell}, E., {Faber}, S., {Ferguson}, H., {Koo}, D., {Bassett}, R., {Bernyk}, M., {Blancato}, K., {Bournaud}, F., {Cassata}, P., {Castellano}, M., {Cheung}, E., {Conselice}, C., {Croton}, D., {Dahlen}, T., , {de Mello}, D., et al. (2015). "{CANDELS Visual Classifications: Scheme, Data Release, and First Results}". apjs, 221, 11.
• {Kelly}, P., {Rodney}, S., {Brammer}, G., {Strolger}, L., {Foley}, R., {Treu}, T., {Zitrin}, A., {Filippenko}, A., {Jha}, S., {Riess}, A., {Hjorth}, J., {Schmidt}, K., {Graur}, O., {Bradac}, M., {Weiner}, B., {Linden}, A., {McCully}, C., {Molino}, A., {Selsing}, J., , {Nonino}, M., et al. (2015). "{Detection of a SN near the center of the galaxy cluster field MACS1149 consistent with predictions of a new image of Supernova Refsdal}". The Astronomer's Telegram, 8402.
• {Kelly}, P., {Rodney}, S., {Treu}, T., {Foley}, R., {Brammer}, G., {Schmidt}, K., {Zitrin}, A., {Sonnenfeld}, A., {Strolger}, L., {Graur}, O., {Filippenko}, A., {Jha}, S., {Riess}, A., {Bradac}, M., {Weiner}, B., {Scolnic}, D., {Malkan}, M., Linden}, A., {Trenti}, M., , {Hjorth}, J., et al. (2015). "{Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens}". Science, 347, 1123-1126.
• {Mei}, S., {Scarlata}, C., {Pentericci}, L., {Newman}, J., {Weiner}, B., {Ashby}, M., {Castellano}, M., {Conselice}, C., {Finkelstein}, S., {Galametz}, A., {Grogin}, N., {Koekemoer}, A., {Huertas-Company}, M., {Lani}, C., {Lucas}, R., {Papovich}, C., {Rafelski}, M., , H. (2015). "{Star-forming Blue ETGs in Two Newly Discovered Galaxy Overdensities in the HUDF at z=1.84 and 1.9: Unveiling the Progenitors of Passive ETGs in Cluster Cores}". apj, 804, 117.
• {Morris}, A., {Kocevski}, D., {Trump}, J., {Weiner}, B., {Hathi}, N., {Barro}, G., {Dahlen}, T., {Faber}, S., {Finkelstein}, S., {Fontana}, A., {Ferguson}, H., {Grogin}, N., {Gr{"u}tzbauch}, R., {Guo}, Y., {Hsu}, L., {Koekemoer}, A., {Koo}, D., {Mobasher}, B., {Pforr}, J., , {Salvato}, M., et al. (2015). "{A WFC3 Grism Emission Line Redshift Catalog in the GOODS-South Field}". aj, 149, 178.
• {Papovich}, C., {Labb{'e}}, I., {Quadri}, R., {Tilvi}, V., {Behroozi}, P., {Bell}, E., {Glazebrook}, K., {Spitler}, L., {Straatman}, C., {Tran}, K., {Cowley}, M., {Dav{'e}}, R., {Dekel}, A., {Dickinson}, M., {Ferguson}, H., {Finkelstein}, S., {Gawiser}, E., {Inami}, H., {Faber}, S., , {Kacprzak}, G., et al. (2015). "{ZFOURGE/CANDELS: On the Evolution of M* Galaxy Progenitors from z = 3 to 0.5}". apj, 803, 26.
• {Popping}, G., {Caputi}, K., {Trager}, S., {Somerville}, R., {Dekel}, A., {Kassin}, S., {Kocevski}, D., {Koekemoer}, A., {Faber}, S., {Ferguson}, H., {Galametz}, A., {Grogin}, N., {Guo}, Y., {Lu}, Y., {Wel}, A., , B. (2015). "{The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 $lt$ z $lt$ 3.0}". mnras, 454, 2258-2276.
• {Santini}, P., {Ferguson}, H., {Fontana}, A., {Mobasher}, B., {Barro}, G., {Castellano}, M., {Finkelstein}, S., {Grazian}, A., {Hsu}, L., {Lee}, B., {Lee}, S., {Pforr}, J., {Salvato}, M., {Wiklind}, T., {Wuyts}, S., {Almaini}, O., {Cooper}, M., {Galametz}, A., {Weiner}, B., , {Amorin}, R., et al. (2015). "{Stellar Masses from the CANDELS Survey: The GOODS-South and UDS Fields}". apj, 801, 97.
• {Simons}, R., {Kassin}, S., {Weiner}, B., {Heckman}, T., {Lee}, J., {Lotz}, J., {Peth}, M., , K. (2015). "{A transition mass in the local Tully-Fisher relation}". mnras, 452, 986-997.
• {Williams}, C., {Giavalisco}, M., {Lee}, B., {Tundo}, E., {Mobasher}, B., {Nayyeri}, H., {Ferguson}, H., {Koekemoer}, A., {Trump}, J., {Cassata}, P., {Dekel}, A., {Guo}, Y., {Lee}, K., {Pentericci}, L., {Bell}, E., {Castellano}, M., {Finkelstein}, S., {Fontana}, A., {Grazian}, A., , {Grogin}, N., et al. (2015). "{The Interstellar Medium and Feedback in the Progenitors of the Compact Passive Galaxies at z ~{} 2}". apj, 800, 21.
• Ahn, C. P., Alexandroff, R., Allende Prieto, C., Anders, F., Anderson, S. F., Anderton, T., Andrews, B. H., Aubourg, '., Bailey, S., Bastien, F. A., & al., e. (2014). The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment. apjs, 211, 17.
• Ahn, C. P., Alexandroff, R., Allende, P. C., Anders, F., Anderson, S. F., Anderton, T., Andrews, B. H., Aubourg, E., Bailey, S., Bastien, F. A., Bautista, J. E., Beers, T. C., Beifiori, A., Bender, C. F., Berlind, A. A., Beutler, F., Bhardwaj, V., Bird, J. C., Bizyaev, D., , Blake, C. H., et al. (2014). THE TENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST SPECTROSCOPIC DATA FROM THE SDSS-III APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 211(2).
• Alberts, S., Pope, A., Brodwin, M., Atlee, D. W., Lin, Y., Dey, A., Eisenhardt, P. R., Gettings, D. P., Gonzalez, A. H., Jannuzi, B. T., Mancone, C. L., Moustakas, J., Snyder, G. F., Stanford, S. A., Stern, D., Weiner, B. J., & Zeimann, G. R. (2014). The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years. mnras, 437, 437-457.
• Alberts, S., Pope, A., Brodwin, M., Atlee, D. W., Lin, Y., Dey, A., Eisenhardt, P., Gettings, D. P., Gonzalez, A. H., Jannuzi, B. T., Mancone, C. L., Moustakas, J., Snyder, G. F., Stanford, S. A., Stern, D., Weiner, B. J., & Zeimann, G. R. (2014). The evolution of dust-obscured star formation activity in galaxy clusters relative to the field over the last 9 billion years. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 437(1), 437-457.
• Buitrago, F., Conselice, C. J., Epinat, B., Bedregal, A. G., Gr "utzbauch, R., & Weiner, B. J. (2014). SINFONI/VLT 3D spectroscopy of massive galaxies: evidence of rotational support at z tilde 1.4. mnras, 439, 1494-1521.
• Buitrago, F., Conselice, C. J., Epinat, B., Bedregal, A. G., Gruetzbauch, R., & Weiner, B. J. (2014). SINFONI/VLT 3D spectroscopy of massive galaxies: evidence of rotational support at z similar to 1.4. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 439(2), 1494-1521.
• Buitrago, F., Conselice, C. J., Epinat, B., Bedregal, A. G., Grutzbauch, R., & Weiner, B. J. (2014). SINFONI/VLT 3D spectroscopy of massive galaxies: Evidence of rotational support at z~1.4.
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  There is cumulative evidence showing that, for the most massive galaxies, thefraction of disk-like objects compared to those with spheroidal propertiesincreases with redshift. However, this evolution is thus far based on thesurface brightness study of these objects. To explore the consistency of thisscenario, it is necessary to measure the dynamical status of these galaxies.With this aim we have obtained seeing-limited near-infrared integral fieldspectra in the H-band for 10 massive galaxies (M_{stellar} >10^{11} h_{70}^-2M_{Sun}) at z~1.4 with SINFONI at the VLT. Our sample is selected by theirstellar mass and EW[OII] > 15 \AA, to secure their kinematic measurements, butwithout accounting for any morphological or flux criteria a priori. Throughthis 3D kinematic spectroscopy analysis we find that half (i.e. 50+/-7%) of ourgalaxies are compatible with being rotationally supported disks, in agreementwith previous morphological expectations. This is a factor of approximately twohigher than what is observed in the present Universe for objects of the samestellar mass. Strikingly, the majority of our sample of massive galaxies showextended and fairly high rotational velocity maps, implying that massivegalaxies acquire rapidly rotational support and hence gravitationalequilibrium. Our sample also show evidence for ongoing interactions andmergers. Summarizing, massive galaxies at high-z show a significant diversityand must have continued evolution beyond the fading of stellar populations, tobecome their present day counterparts.[Journal_ref: ]
• Decarli, R., Walter, F., Carilli, C., Riechers, D., Cox, P., Neri, R., Aravena, M., Bell, E., Bertoldi, F., Colombo, D., Da Cunha, E., Daddi, E., Dickinson, M., Downes, D., Ellis, R., Lentati, L., Maiolino, R., Menten, K. M., Rix, H., , Sargent, M., et al. (2014). A Molecular Line Scan in the Hubble Deep Field North. apj, 782, 78.
• Dolley, T., Brown, M. J., Weiner, B. J., Brodwin, M., Kochanek, C. S., Pimbblet, K. A., Palamara, D. P., Jannuzi, B. T., Dey, A., Atlee, D. W., & Beare, R. (2014). THE CLUSTERING AND HALO MASSES OF STAR-FORMING GALAXIES AT z < 1. ASTROPHYSICAL JOURNAL, 797(2).
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  We present clustering measurements and halo masses of star-forming galaxies at 0.2 < z < 1.0. After excluding active galactic nuclei (AGNs), we construct a sample of 22,553 24 mu m sources selected from 8.42 deg(2) of the Spitzer MIPS AGN and Galaxy Evolution Survey of Bootes. Mid-infrared imaging allows us to observe galaxies with the highest star formation rates (SFRs), less biased by dust obscuration afflicting the optical bands. We find that the galaxies with the highest SFRs have optical colors that are redder than typical blue cloud galaxies, with many residing within the green valley. At z > 0.4 our sample is dominated by luminous infrared galaxies (LIRGs, L-TIR > 10(11) L-circle plus) and is composed entirely of LIRGs and ultraluminous infrared galaxies (ULIRGs, L-TIR > 10(12) L-circle plus) at z > 0.6. We observe weak clustering of r(0) approximate to 3-6 h(-1) Mpc for almost all of our star-forming samples. We find that the clustering and halo mass depend on L-TIR at all redshifts, where galaxies with higher LTIR (hence higher SFRs) have stronger clustering. Galaxies with the highest SFRs at each redshift typically reside within dark matter halos of M-halo approximate to 10(12.9) h(-1) M-circle plus. This is consistent with a transitional halo mass, above which star formation is largely truncated, although we cannot exclude that ULIRGs reside within higher mass halos. By modeling the clustering evolution of halos, we connect our star-forming galaxy samples to their local descendants. Most star-forming galaxies at z < 1.0 are the progenitors of L less than or similar to 2.5L(*) blue galaxies in the local universe, but star-forming galaxies with the highest SFRs (L-TIR greater than or similar to 10(11.7) L-circle plus) at 0.6 < z < 1.0 are the progenitors of early-type galaxies in denser group environments.
• Goulding, A. D., Forman, W. R., Hickox, R. C., Jones, C., Murray, S. S., Paggi, A., Ashby, M. L., Coil, A. L., Cooper, M. C., Huang, J., Kraft, R., Newman, J. A., Weiner, B. J., & Willner, S. P. (2014). Tracing the Evolution of Active Galactic Nuclei Host Galaxies over the Last 9 Gyr of Cosmic Time. apj, 783, 40.
• Kassin, S. A., Brooks, A., Governato, F., Weiner, B. J., & Gardner, J. P. (2014). KINEMATIC EVOLUTION OF SIMULATED STAR-FORMING GALAXIES. ASTROPHYSICAL JOURNAL, 790(2).
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  Recent observations have shown that star-forming galaxies like our own Milky Way evolve kinematically into ordered thin disks over the last similar to 8 billion years since z = 1.2, undergoing a process of "disk settling." For the first time, we study the kinematic evolution of a suite of four state of the art "zoom in" hydrodynamic simulations of galaxy formation and evolution in a fully cosmological context and compare with these observations. Until now, robust measurements of the internal kinematics of simulated galaxies were lacking because the simulations suffered from low resolution, overproduction of stars, and overly massive bulges. The current generation of simulations has made great progress in overcoming these difficulties and is ready for a kinematic analysis. We show that simulated galaxies follow the same kinematic trends as real galaxies: they progressively decrease in disordered motions (sigma(g)) and increase in ordered rotation (V-rot) with time. The slopes of the relations between both sigma(g) and V-rot with redshift are consistent between the simulations and the observations. In addition, the morphologies of the simulated galaxies become less disturbed with time, also consistent with observations. This match between the simulated and observed trends is a significant success for the current generation of simulations, and a first step in determining the physical processes behind disk settling.
• Kassin, S. A., Brooks, A., Governato, F., Weiner, B. J., & Gardner, J. P. (2014). Kinematic Evolution of Simulated Star-Forming Galaxies.
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  Recent observations have shown that star-forming galaxies like our own MilkyWay evolve kinematically into ordered thin disks over the last ~8 billion yearssince z=1.2, undergoing a process of "disk settling." For the first time, westudy the kinematic evolution of a suite of four state of the art "zoom in"hydrodynamic simulations of galaxy formation and evolution in a fullycosmological context and compare with these observations. Until now, robustmeasurements of the internal kinematics of simulated galaxies were lacking asthe simulations suffered from low resolution, overproduction of stars, andoverly massive bulges. The current generation of simulations has made greatprogress in overcoming these difficulties and is ready for a kinematicanalysis. We show that simulated galaxies follow the same kinematic trends asreal galaxies: they progressively decrease in disordered motions (sigma_g) andincrease in ordered rotation (Vrot) with time. The slopes of the relationsbetween both sigma_g and Vrot with redshift are consistent between thesimulations and the observations. In addition, the morphologies of thesimulated galaxies become less disturbed with time, also consistent withobservations, and they both have similarly large scatter. This match betweenthe simulated and observed trends is a significant success for the currentgeneration of simulations, and a first step in determining the physicalprocesses behind disk settling.[Journal_ref: ]
• Newman, S. F., Buschkamp, P., Genzel, R., Schreiber, N. M., Kurk, J., Sternberg, A., Gnat, O., Rosario, D., Mancini, C., Lilly, S. J., Renzini, A., Burkert, A., Carollo, C. M., Cresci, G., Davies, R., Eisenhauer, F., Genel, S., Shapiro Griffin, K., Hicks, E. K., , Lutz, D., et al. (2014). Nebular Excitation in z ~ 2 Star-forming Galaxies from the SINS and LUCI Surveys: The Influence of Shocks and Active Galactic Nuclei. apj, 781, 21.
• Newman, S. F., Buschkamp, P., Genzel, R., Schreiber, N., Kurk, J., Sternberg, A., Gnat, O., Rosario, D., Mancini, C., Lilly, S. J., Renzini, A., Burkert, A., Carollo, C. M., Cresci, G., Davies, R., Eisenhauer, F., Genel, S., Griffin, K. S., Hicks, E., , Lutz, D., et al. (2014). NEBULAR EXCITATION IN z similar to 2 STAR-FORMING GALAXIES FROM THE SINS AND LUCI SURVEYS: THE INFLUENCE OF SHOCKS AND ACTIVE GALACTIC NUCLEI. ASTROPHYSICAL JOURNAL, 781(1).
• Rodney, S. A., Riess, A. G., Strolger, L., Dahlen, T., Graur, O., Casertano, S., Dickinson, M. E., Ferguson, H. C., Garnavich, P., Hayden, B., Jha, S. W., Jones, D. O., Kirshner, R. P., Koekemoer, A. M., McCully, C., Mobasher, B., Patel, B., Weiner, B. J., Cenko, S. B., , Clubb, K. I., et al. (2014). TYPE Ia SUPERNOVA RATE MEASUREMENTS TO REDSHIFT 2.5 FROM CANDELS: SEARCHING FOR PROMPT EXPLOSIONS IN THE EARLY UNIVERSE. ASTRONOMICAL JOURNAL, 148(1).
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  dThe Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) was a multi-cycle treasury program on the Hubble Space Telescope (HST) that surveyed a total area of -0.25 deg2 with -900 HST orbits spread across five fields over three years. Within these survey images we discovered 65 supernovae (SNe) of all types, out to z 2.5. We classify -24 of these as Type Ia SNe (SNe Ia) based on host galaxy redshifts and SN photometry (supplemented by grism spectroscopy of six SNe). Here we present a measurement of the volumetric SN Ia rate as a function of redshift, reaching for the first time beyond z =- 2 and putting new constraints on SN Ia progenitor models. Our highest redshift bin includes detections of SNe that exploded when the universe was only -3 Gyr old and near the peak of the cosmic star formation history. This gives the CANDELS high redshift sample unique leverage for evaluating the fraction of SNe Ia that explode promptly after formation (
• Trump, J. R., Barro, G., Juneau, S., Weiner, B. J., Luo, B., Brammer, G. B., Bell, E. F., Brandt, W. N., Dekel, A., Guo, Y., Hopkins, P. F., Koo, D. C., Kocevski, D. D., McIntosh, D. H., Momcheva, I., Faber, S. M., Ferguson, H. C., Grogin, N. A., Kartaltepe, J., , Koekemoer, A. M., et al. (2014). NO MORE ACTIVE GALACTIC NUCLEI IN CLUMPY DISKS THAN IN SMOOTH GALAXIES AT z similar to 2 IN CANDELS/3D-HST. ASTROPHYSICAL JOURNAL, 793(2).
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  We use CANDELS imaging, 3D-HST spectroscopy, and Chandra X-ray data to investigate if active galactic nuclei (AGNs) are preferentially fueled by violent disk instabilities funneling gas into galaxy centers at 1.3 < z < 2.4. We select galaxies undergoing gravitational instabilities using the number of clumps and degree of patchiness as proxies. The CANDELS visual classification system is used to identify 44 clumpy disk galaxies, along with mass-matched comparison samples of smooth and intermediate morphology galaxies. We note that despite being mass-matched and having similar star formation rates, the smoother galaxies tend to be smaller disks with more prominent bulges compared to the clumpy galaxies. The lack of smooth extended disks is probably a general feature of the z similar to 2 galaxy population, and means we cannot directly compare with the clumpy and smooth extended disks observed at lower redshift. We find that z similar to 2 clumpy galaxies have slightly enhanced AGN fractions selected by integrated line ratios (in the mass-excitation method), but the spatially resolved line ratios indicate this is likely due to extended phenomena rather than nuclear AGNs. Meanwhile, the X-ray data show that clumpy, smooth, and intermediate galaxies have nearly indistinguishable AGN fractions derived from both individual detections and stacked non-detections. The data demonstrate that AGN fueling modes at z similar to 1.85-whether violent disk instabilities or secular processes-are as efficient in smooth galaxies as they are in clumpy galaxies.
• Walter, F., Decarli, R., Sargent, M., Carilli, C., Dickinson, M., Riechers, D., Ellis, R., Stark, D., Weiner, B., Aravena, M., Bell, E., Bertoldi, F., Cox, P., Da Cunha, E., Daddi, E., Downes, D., Lentati, L., Maiolino, R., Menten, K. M., , Neri, R., et al. (2014). A Molecular Line Scan in the Hubble Deep Field North: Constraints on the CO Luminosity Function and the Cosmic H$_2$ Density. apj, 782, 79.
• Ashby, M. L., Willner, S. P., Fazio, G. G., Huang, J., Arendt, R., Barmby, P., Barro, G., Bell, E. F., Bouwens, R., Cattaneo, A., Croton, D., Dav 'e, R., Dunlop, J. S., Egami, E., Faber, S., Finlator, K., Grogin, N. A., Guhathakurta, P., Hernquist, L., , Hora, J. L., et al. (2013). SEDS: The Spitzer Extended Deep Survey. Survey Design, Photometry, and Deep IRAC Source Counts. apj, 769, 80.
• Ashby, M., Willner, S. P., Fazio, G. G., Huang, J. -., Arendt, R., Barmby, P., Barro, G., Bell, E. F., Bouwens, R., Cattaneo, A., Croton, D., Dave, R., Dunlop, J. S., Egami, E., Faber, S., Finlator, K., Grogin, N. A., Guhathakurta, P., Hernquist, L., , Hora, J. L., et al. (2013). SEDS: THE SPITZER EXTENDED DEEP SURVEY. SURVEY DESIGN, PHOTOMETRY, AND DEEP IRAC SOURCE COUNTS. ASTROPHYSICAL JOURNAL, 769(1).
• Cooper, M. C., Yan, R., Dickinson, M., Juneau, S., Lotz, J. M., Newman, J. A., Papovich, C., Salim, S., Walth, G., Weiner, B. J., & Willmer, C. N. (2013). Arizona CDFS Environment Survey, ACES (Cooper+, 2012). VizieR Online Data Catalog, 742, 52116.
• Dahlen, T., Mobasher, B., Faber, S. M., Ferguson, H. C., Barro, G., Finkelstein, S. L., Finlator, K., Fontana, A., Gruetzbauch, R., Johnson, S., Pforr, J., Salvato, M., Wiklind, T., Wuyts, S., Acquaviva, V., Dickinson, M. E., Guo, Y., Huang, J., Huang, K., , Newman, J. A., et al. (2013). A CRITICAL ASSESSMENT OF PHOTOMETRIC REDSHIFT METHODS: A CANDELS INVESTIGATION. ASTROPHYSICAL JOURNAL, 775(2).
• Dahlen, T., Mobasher, B., Faber, S. M., Ferguson, H. C., Barro, G., Finkelstein, S. L., Finlator, K., Fontana, A., Gruetzbauch, R., Johnson, S., Pforr, J., Salvato, M., Wiklind, T., Wuyts, S., Acquaviva, V., Dickinson, M. E., Guo, Y., Huang, J., Huang, K., , Newman, J. A., et al. (2013). A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation. apj, 775, 93.
• Dawson, K. S., Schlegel, D. J., Ahn, C. P., Anderson, S. F., Aubourg, '., Bailey, S., Barkhouser, R. H., Bautista, J. E., Beifiori, A., Berlind, A. A., Bhardwaj, V., Bizyaev, D., Blake, C. H., Blanton, M. R., Blomqvist, M., Bolton, A. S., Borde, A., Bovy, J., Brandt, W. N., , Brewington, H., et al. (2013). The Baryon Oscillation Spectroscopic Survey of SDSS-III. aj, 145, 10.
• Dawson, K. S., Schlegel, D. J., Ahn, C. P., Anderson, S. F., Aubourg, E., Bailey, S., Barkhouser, R. H., Bautista, J. E., Beifiori, A., Berlind, A. A., Bhardwaj, V., Bizyaev, D., Blake, C. H., Blanton, M. R., Blomqvist, M., Bolton, A. S., Borde, A., Bovy, J. o., Brandt, W. N., , Brewington, H., et al. (2013). THE BARYON OSCILLATION SPECTROSCOPIC SURVEY OF SDSS-III. ASTRONOMICAL JOURNAL, 145(1).
• Finkelstein, S. L., Papovich, C., Dickinson, M., Song, M., Tilvi, V., Koekemoer, A. M., Finkelstein, K. D., Mobasher, B., Ferguson, H. C., Giavalisco, M., Reddy, N., Ashby, M. L., Dekel, A., Fazio, G. G., Fontana, A., Grogin, N. A., Huang, J., Kocevski, D., Rafelski, M., , Weiner, B. J., et al. (2013). A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51. nat, 502, 524-527.
• Finkelstein, S. L., Papovich, C., Dickinson, M., Song, M., Tilvi, V., Koekemoer, A. M., Finkelstein, K. D., Mobasher, B., Ferguson, H. C., Giavalisco, M., Reddy, N., Ashby, M., Dekel, A., Fazio, G. G., Fontana, A., Grogin, N. A., Huang, J. -., Kocevski, D., Rafelski, M., , Weiner, B. J., et al. (2013). A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51. NATURE, 502(7472), 524-527.
• Freundlich, J., Combes, F., Tacconi, L. J., Cooper, M. C., Genzel, R., Neri, R., Bolatto, A., Bournaud, F., Burkert, A., Cox, P., Davis, M., Schreiber, N. M., Garcia-Burillo, S., Gracia-Carpio, J., Lutz, D., Naab, T., Newman, S., Sternberg, A., & Weiner, B. (2013). Towards a resolved Kennicutt-Schmidt law at high redshift. aap, 553, A130.
• Galametz, A., Grazian, A., Fontana, A., Ferguson, H. C., Ashby, M. L., Barro, G., Castellano, M., Dahlen, T., Donley, J. L., Faber, S. M., Grogin, N., Guo, Y., Huang, K., Kocevski, D. D., Koekemoer, A. M., Lee, K., McGrath, E. J., Peth, M., Willner, S. P., , Almaini, O., et al. (2013). CANDELS Multiwavelength Catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-deep Survey Field. apjs, 206, 10.
• Galametz, A., Grazian, A., Fontana, A., Ferguson, H. C., Ashby, M., Barro, G., Castellano, M., Dahlen, T., Donley, J. L., Faber, S. M., Grogin, N., Guo, Y., Huang, K., Kocevski, D. D., Koekemoer, A. M., Lee, K., McGrath, E. J., Peth, M., Willner, S. P., , Almaini, O., et al. (2013). CANDELS MULTIWAVELENGTH CATALOGS: SOURCE IDENTIFICATION AND PHOTOMETRY IN THE CANDELS UKIDSS ULTRA-DEEP SURVEY FIELD. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 206(2).
• Genzel, R., Tacconi, L. J., Kurk, J., Wuyts, S., Combes, F., Freundlich, J., Bolatto, A., Cooper, M. C., Neri, R., Nordon, R., Bournaud, F., Burkert, A., Comerford, J., Cox, P., Davis, M., Schreiber, N. M., Garc ' ia-Burillo, S., Gracia-Carpio, J., Lutz, D., , Naab, T., et al. (2013). Phibss: Molecular Gas, Extinction, Star Formation, and Kinematics in the z = 1.5 Star- forming Galaxy EGS13011166. apj, 773, 68.
• Huang, J., Faber, S. M., Willmer, C. N., Rigopoulou, D., Koo, D., Newman, J., Shu, C., Ashby, M. L., Barmby, P., Coil, A., Luo, Z., Magdis, G., Wang, T., Weiner, B., Willner, S. P., Zheng, X. Z., & Fazio, G. G. (2013). Multi-Wavelength Study of a Complete IRAC 3.6 $ mu$m Selected Galaxy Sample: A Fair Census of Red and Blue Populations at Redshifts 0.4-1.2. apj, 766, 21.
• Jones, D. O., Rodney, S. A., Riess, A. G., Mobasher, B., Dahlen, T., McCully, C., Frederiksen, T. F., Casertano, S., Hjorth, J., Keeton, C. R., Koekemoer, A., Strolger, L., Wiklind, T. G., Challis, P., Graur, O. r., Hayden, B., Patel, B., Weiner, B. J., Filippenko, A. V., , Garnavich, P., et al. (2013). THE DISCOVERY OF THE MOST DISTANT KNOWN TYPE Ia SUPERNOVA AT REDSHIFT 1.914. ASTROPHYSICAL JOURNAL, 768(2).
• Jones, D. O., Rodney, S. A., Riess, A. G., Mobasher, B., Dahlen, T., McCully, C., Frederiksen, T. F., Casertano, S., Hjorth, J., Keeton, C. R., Koekemoer, A., Strolger, L., Wiklind, T. G., Challis, P., Graur, O., Hayden, B., Patel, B., Weiner, B. J., Filippenko, A. V., , Garnavich, P., et al. (2013). The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914. apj, 768, 166.
• Juneau, S., Dickinson, M., Bournaud, F., Alexander, D. M., Daddi, E., Mullaney, J. R., Magnelli, B., Kartaltepe, J. S., Hwang, H. S., Willner, S. P., Coil, A. L., Rosario, D. J., Trump, J. R., Weiner, B. J., Willmer, C. N., Cooper, M. C., Elbaz, D., Faber, S. M., Frayer, D. T., , Kocevski, D. D., et al. (2013). Widespread and Hidden Active Galactic Nuclei in Star-forming Galaxies at Redshift gt 0.3. apj, 764, 176.
• Juneau, S., Dickinson, M., Bournaud, F., Alexander, D. M., Daddi, E., Mullaney, J. R., Magnelli, B., Kartaltepe, J. S., Hwang, H. S., Willner, S. P., Coil, A. L., Rosario, D. J., Trump, J. R., Weiner, B. J., Willmer, C., Cooper, M. C., Elbaz, D., Faber, S. M., Frayer, D. T., , Kocevski, D. D., et al. (2013). WIDESPREAD AND HIDDEN ACTIVE GALACTIC NUCLEI IN STAR-FORMING GALAXIES AT REDSHIFT > 0.3. ASTROPHYSICAL JOURNAL, 764(2).
• Kornei, K. A., Shapley, A. E., Martin, C. L., Coil, A. L., Lotz, J. M., & Weiner, B. J. (2013). FINE-STRUCTURE Fe II* EMISSION AND RESONANT Mg II EMISSION IN z similar to 1 STAR-FORMING GALAXIES. ASTROPHYSICAL JOURNAL, 774(1).
• Kornei, K. A., Shapley, A. E., Martin, C. L., Coil, A. L., Lotz, J. M., & Weiner, B. J. (2013). Fine-structure Fe II* Emission and Resonant Mg II Emission in z ~ 1 Star-forming Galaxies. apj, 774, 50.
• Maseda, M. V., Wel, A., Cunha, E., Rix, H., Pacifici, C., Momcheva, I., Brammer, G. B., Franx, M., Dokkum, P., Bell, E. F., Fumagalli, M., Grogin, N. A., Kocevski, D. D., Koekemoer, A. M., Lundgren, B. F., Marchesini, D., Nelson, E. J., Patel, S. G., Skelton, R. E., , Straughn, A. N., et al. (2013). Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z ~ 2. apjl, 778, L22.
• Maseda, M. V., van, d., da, C. E., Rix, H., Pacifici, C., Momcheva, I., Brammer, G. B., Franx, M., van, D. P., Bell, E. F., Fumagalli, M., Grogin, N. A., Kocevski, D. D., Koekemoer, A. M., Lundgren, B. F., Marchesini, D., Nelson, E. J., Patel, S. G., Skelton, R. E., , Straughn, A. N., et al. (2013). CONFIRMATION OF SMALL DYNAMICAL AND STELLAR MASSES FOR EXTREME EMISSION LINE GALAXIES AT z similar to 2. ASTROPHYSICAL JOURNAL LETTERS, 778(1).
• Mostek, N., Coil, A. L., Cooper, M., Davis, M., Newman, J. A., & Weiner, B. J. (2013). THE DEEP2 GALAXY REDSHIFT SURVEY: CLUSTERING DEPENDENCE ON GALAXY STELLAR MASS AND STAR FORMATION RATE AT z similar to 1. ASTROPHYSICAL JOURNAL, 767(1).
• Mostek, N., Coil, A. L., Cooper, M., Davis, M., Newman, J. A., & Weiner, B. J. (2013). The DEEP2 Galaxy Redshift Survey: Clustering Dependence on Galaxy Stellar Mass and Star Formation Rate at z ~ 1. apj, 767, 89.
• Newman, J. A., Cooper, M. C., Davis, M., Faber, S. M., Coil, A. L., Guhathakurta, P., Koo, D. C., Phillips, A. C., Conroy, C., Dutton, A. A., Finkbeiner, D. P., Gerke, B. F., Rosario, D. J., Weiner, B. J., Willmer, C. N., Yan, R., Harker, J. J., Kassin, S. A., Konidaris, N. P., , Lai, K., et al. (2013). The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts. apjs, 208, 5.
• Newman, J. A., Cooper, M. C., Davis, M., Faber, S. M., Coil, A. L., Guhathakurta, P., Koo, D. C., Phillips, A. C., Conroy, C., Dutton, A. A., Finkbeiner, D. P., Gerke, B. F., Rosario, D. J., Weiner, B. J., Willmer, C., Yan, R., Harker, J. J., Kassin, S. A., Konidaris, N. P., , Lai, K., et al. (2013). THE DEEP2 GALAXY REDSHIFT SURVEY: DESIGN, OBSERVATIONS, DATA REDUCTION, AND REDSHIFTS. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 208(1).
• Pacifici, C., Kassin, S. A., Weiner, B., Charlot, S., & Gardner, J. P. (2013). THE RISE AND FALL OF THE STAR FORMATION HISTORIES OF BLUE GALAXIES AT REDSHIFTS 0.2 < z < 1.4. ASTROPHYSICAL JOURNAL LETTERS, 762(1).
• Pacifici, C., Kassin, S. A., Weiner, B., Charlot, S., & Gardner, J. P. (2013). The Rise and Fall of the Star Formation Histories of Blue Galaxies at Redshifts 0.2 lt z lt 1.4. apjl, 762, L15.
• Pacifici, C., Kassin, S. A., Weiner, B., Charlot, S., & Gardner, J. P. (2013). The rise and fall of the star formation histories of blue galaxies at redshifts 0.2
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  Popular cosmological scenarios predict that galaxies form hierarchically fromthe merger of many progenitors, each with their own unique star formationhistory (SFH). We use a sophisticated approach to constrain the SFHs of 4517blue (presumably star-forming) galaxies with spectroscopic redshifts in therange 0.2 < z < 1.4 from the All-Wavelength Extended Groth Strip InternationalSurvey (AEGIS). This consists in the Bayesian analysis of the observed galaxyspectral energy distributions with a comprehensive library of synthetic spectraassembled using realistic, hierarchical star formation and chemical enrichmenthistories from cosmological simulations. We constrain the SFH of each galaxy inour sample by comparing the observed fluxes in the B, R, I and Ks bands andrest-frame optical emission-line luminosities with those of one million modelspectral energy distributions. We explore the dependence of the resulting SFHson galaxy stellar mass and redshift. We find that the average SFHs of high-massgalaxies rise and fall in a roughly symmetric bell-shaped manner, while thoseof low-mass galaxies rise progressively in time, consistent with the typicallystronger activity of star formation in low-mass compared to high-mass galaxies.For galaxies of all masses, the star formation activity rises more rapidly athigh than at low redshift. These findings imply that the standard approximationof exponentially declining SFHs widely used to interpret observed galaxyspectral energy distributions may not be appropriate to constrain the physicalparameters of star-forming galaxies at intermediate redshifts.[Journal_ref: ]
• Palamara, D. P., Brown, M. J., Jannuzi, B. T., Dey, A., Stern, D., Pimbblet, K. A., Weiner, B. J., Ashby, M. L., Kochanek, C. S., Gonzalez, A., Brodwin, M., Le Floc'h, E., & Rieke, M. (2013). The Clustering of Extremely Red Objects. apj, 764, 31.
• Palamara, D. P., Brown, M., Jannuzi, B. T., Dey, A., Stern, D., Pimbblet, K. A., Weiner, B. J., Ashby, M., Kochanek, C. S., Gonzalez, A., Brodwin, M., Le, F. E., & Rieke, M. (2013). THE CLUSTERING OF EXTREMELY RED OBJECTS. ASTROPHYSICAL JOURNAL, 764(1).
• Rujopakarn, W., Rieke, G. H., Weiner, B. J., 'alez, P., Rex, M., Walth, G. L., & Kartaltepe, J. S. (2013). Mid-infrared Determination of Total Infrared Luminosity and Star Formation Rates of Local and High-redshift Galaxies. apj, 767, 73.
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• Comerford, J. M., Gerke, B. F., Stern, D., Cooper, M. C., Weiner, B. J., Newman, J. A., Madsen, K., & Barrows, R. S. (2012). Kiloparsec-scale Spatial Offsets in Double-peaked Narrow-line Active Galactic Nuclei. I. Markers for Selection of Compelling Dual Active Galactic Nucleus Candidates. apj, 753, 42.
• Cooper, M. C., Griffith, R. L., Newman, J. A., Coil, A. L., Davis, M., Dutton, A. A., Faber, S. M., Guhathakurta, P., Koo, D. C., Lotz, J. M., Weiner, B. J., Willmer, C. N., & Yan, R. (2012). The DEEP3 Galaxy Redshift Survey: the impact of environment on the size evolution of massive early-type galaxies at intermediate redshift. mnras, 419, 3018-3027.
• Cooper, M. C., Griffith, R. L., Newman, J. A., Coil, A. L., Davis, M., Dutton, A. A., Faber, S. M., Guhathakurta, P., Koo, D. C., Lotz, J. M., Weiner, B. J., Willmer, C., & Yan, R. (2012). The DEEP3 Galaxy Redshift Survey: the impact of environment on the size evolution of massive early-type galaxies at intermediate redshift. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 419(4), 3018-3027.
• Cooper, M. C., Yan, R., Dickinson, M., Juneau, S., Lotz, J. M., Newman, J. A., Papovich, C., Salim, S., Walth, G., Weiner, B. J., & Willmer, C. (2012). The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS Spectroscopic Survey of the Chandra Deep Field-South. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 425(3), 2116-2127.
• Cooper, M. C., Yan, R., Dickinson, M., Juneau, S., Lotz, J. M., Newman, J. A., Papovich, C., Salim, S., Walth, G., Weiner, B. J., & Willmer, C. N. (2012). The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS Spectroscopic Survey of the Chandra Deep Field-South. mnras, 425, 2116-2127.
• Genzel, R., Tacconi, L. J., Combes, F., Bolatto, A., Neri, R., Sternberg, A., Cooper, M. C., Bouch 'e, N., Bournaud, F., Burkert, A., Comerford, J., Cox, P., Davis, M., Schreiber, N. M., Garcia-Burillo, S., Gracia-Carpio, J., Lutz, D., Naab, T., Newman, S., , Saintonge, A., et al. (2012). The Metallicity Dependence of the CO rarr H$_2$ Conversion Factor in z gt= 1 Star-forming Galaxies. apj, 746, 69.
• Genzel, R., Tacconi, L. J., Combes, F., Bolatto, A., Neri, R., Sternberg, A., Cooper, M. C., Bouche, N., Bournaud, F., Burkert, A., Comerford, J., Cox, P., Davis, M., Schreiber, N., Garcia-Burillo, S., Gracia-Carpio, J., Lutz, D., Naab, T., Newman, S., , Saintonge, A., et al. (2012). THE METALLICITY DEPENDENCE OF THE CO -> H-2 CONVERSION FACTOR IN z >= 1 STAR-FORMING GALAXIES. ASTROPHYSICAL JOURNAL, 746(1).
• Gerke, B. F., Newman, J. A., Davis, M., Coil, A. L., Cooper, M. C., Dutton, A. A., Faber, S. M., Guhathakurta, P., Konidaris, N., Koo, D. C., Lin, L., Noeske, K., Phillips, A. C., Rosario, D. J., Weiner, B. J., Willmer, C. N., & Yan, R. (2012). The DEEP2 Galaxy Redshift Survey: The Voronoi-Delaunay Method Catalog of Galaxy Groups. apj, 751, 50.
• Gerke, B. F., Newman, J. A., Davis, M., Coil, A. L., Cooper, M. C., Dutton, A. A., Faber, S. M., Guhathakurta, P., Konidaris, N., Koo, D. C., Lin, L., Noeske, K., Phillips, A. C., Rosario, D. J., Weiner, B. J., Willmer, C., & Yan, R. (2012). THE DEEP2 GALAXY REDSHIFT SURVEY: THE VORONOI-DELAUNAY METHOD CATALOG OF GALAXY GROUPS. ASTROPHYSICAL JOURNAL, 751(1).
• Griffith, R. L., Cooper, M. C., Newman, J. A., Moustakas, L. A., Stern, D., Comerford, J. M., Davis, M., Lotz, J. M., Barden, M., Conselice, C. J., Capak, P. L., Faber, S. M., Kirkpatrick, J. D., Koekemoer, A. M., Koo, D. C., Noeske, K. G., Scoville, N., Sheth, K., Shopbell, P., , Willmer, C. N., et al. (2012). The Advanced Camera for Surveys General Catalog: Structural Parameters for Approximately Half a Million Galaxies. apjs, 200, 9.
• Griffith, R. L., Cooper, M. C., Newman, J. A., Moustakas, L. A., Stern, D., Comerford, J. M., Davis, M., Lotz, J. M., Barden, M., Conselice, C. J., Capak, P. L., Faber, S. M., Kirkpatrick, J. D., Koekemoer, A. M., Koo, D. C., Noeske, K. G., Scoville, N., Sheth, K., Shopbell, P., , Willmer, C., et al. (2012). THE ADVANCED CAMERA FOR SURVEYS GENERAL CATALOG: STRUCTURAL PARAMETERS FOR APPROXIMATELY HALF A MILLION GALAXIES. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 200(1).
• Kartaltepe, J. S., Dickinson, M., Alexander, D. M., Bell, E. F., Dahlen, T., Elbaz, D., Faber, S. M., Lotz, J., McIntosh, D. H., Wiklind, T., Altieri, B., Aussel, H., Bethermin, M., Bournaud, F., Charmandaris, V., Conselice, C. J., Cooray, A., Dannerbauer, H., Dav 'e, R., , Dunlop, J., et al. (2012). GOODS-Herschel and CANDELS: The Morphologies of Ultraluminous Infrared Galaxies at z ~ 2. apj, 757, 23.
• Kartaltepe, J. S., Dickinson, M., Alexander, D. M., Bell, E. F., Dahlen, T., Elbaz, D., Faber, S. M., Lotz, J., McIntosh, D. H., Wiklind, T., Altieri, B., Aussel, H., Bethermin, M., Bournaud, F., Charmandaris, V., Conselice, C. J., Cooray, A., Dannerbauer, H., Dave, R., , Dunlop, J., et al. (2012). GOODS-HERSCHEL AND CANDELS: THE MORPHOLOGIES OF ULTRALUMINOUS INFRARED GALAXIES AT z similar to 2. ASTROPHYSICAL JOURNAL, 757(1).
• Kassin, S. A., Weiner, B. J., Faber, S. M., Gardner, J. P., Willmer, C. N., Coil, A. L., Cooper, M. C., Devriendt, J., Dutton, A. A., Guhathakurta, P., Koo, D. C., Metevier, A. J., Noeske, K. G., & Primack, J. R. (2012). The Epoch of Disk Settling: z ~ 1 to Now. apj, 758, 106.
• Kassin, S. A., Weiner, B. J., Faber, S. M., Gardner, J. P., Willmer, C., Coil, A. L., Cooper, M. C., Devriendt, J., Dutton, A. A., Guhathakurta, P., Koo, D. C., Metevier, A. J., Noeske, K. G., & Primack, J. R. (2012). THE EPOCH OF DISK SETTLING: z similar to 1 TO NOW. ASTROPHYSICAL JOURNAL, 758(2).
• Ko, J., Im, M., Lee, H. M., Lee, M. G., Kim, S. J., Shim, H., Jeon, Y., Hwang, H. S., Willmer, C. N., Malkan, M. A., Papovich, C., Weiner, B. J., Matsuhara, H., Oyabu, S., & Takagi, T. (2012). AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: Mid- infrared View of Transition Galaxies. apj, 745, 181.
• Ko, J., Im, M., Lee, H. M., Lee, M. G., Kim, S. J., Shim, H., Jeon, Y., Hwang, H. S., Willmer, C., Malkan, M. A., Papovich, C., Weiner, B. J., Matsuhara, H., Oyabu, S., & Takagi, T. (2012). AKARI OBSERVATION OF THE NORTH ECLIPTIC POLE (NEP) SUPERCLUSTER AT z=0.087: MID-INFRARED VIEW OF TRANSITION GALAXIES. ASTROPHYSICAL JOURNAL, 745(2).
• Martin, C. L., Shapley, A. E., Coil, A. L., Kornei, K. A., Bundy, K., Weiner, B. J., Noeske, K. G., & Schiminovich, D. (2012). DEMOGRAPHICS AND PHYSICAL PROPERTIES OF GAS OUTFLOWS/INFLOWS AT 0.4 < z < 1.4. ASTROPHYSICAL JOURNAL, 760(2).
• Martin, C. L., Shapley, A. E., Coil, A. L., Kornei, K. A., Bundy, K., Weiner, B. J., Noeske, K. G., & Schiminovich, D. (2012). Demographics and Physical Properties of Gas Outflows/Inflows at 0.4 lt z lt 1.4. apj, 760, 127.
• Mostek, N., Coil, A. L., Moustakas, J., Salim, S., & Weiner, B. J. (2012). CALIBRATING THE STAR FORMATION RATE AT z similar to 1 FROM OPTICAL DATA. ASTROPHYSICAL JOURNAL, 746(2).
• Mostek, N., Coil, A. L., Moustakas, J., Salim, S., & Weiner, B. J. (2012). Calibrating the Star Formation Rate at z ~ 1 from Optical Data. apj, 746, 124.
• Mostek, N., Coil, A. L., Moustakas, J., Salim, S., & Weiner, B. J. (2012). Calibrating the Star Formation Rate at z=1 from Optical Data. ApJ,.
  More info

  We present a star-formation rate calibration based on optical data that isconsistent with average observed rates in both the red and blue galaxypopulations at z~1. The motivation for this study is to calculate SFRs forDEEP2 Redshift Survey galaxies in the 0.7
• Nidever, D. L., Zasowski, G., Majewski, S. R., Bird, J., Robin, A. C., Martinez-Valpuesta, I., Beaton, R. L., Sch "onrich, R., Schultheis, M., Wilson, J. C., Skrutskie, M. F., O'Connell, R. W., Shetrone, M., Schiavon, R. P., Johnson, J. A., Weiner, B., Gerhard, O., Schneider, D. P., Allende Prieto, C., , Sellgren, K., et al. (2012). The Apache Point Observatory Galactic Evolution Experiment: First Detection of High- velocity Milky Way Bar Stars. apjl, 755, L25.
• Nidever, D. L., Zasowski, G., Majewski, S. R., Bird, J., Robin, A. C., Martinez-Valpuesta, I., Beaton, R. L., Schoenrich, R., Schultheis, M., Wilson, J. C., Skrutskie, M. F., O'Connell, R. W., Shetrone, M., Schiavon, R. P., Johnson, J. A., Weiner, B., Gerhard, O., Schneider, D. P., Prieto, C. A., , Sellgren, K., et al. (2012). THE APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT: FIRST DETECTION OF HIGH-VELOCITY MILKY WAY BAR STARS. ASTROPHYSICAL JOURNAL LETTERS, 755(2).
• Ono, Y., Ouchi, M., Mobasher, B., Dickinson, M., Penner, K., Shimasaku, K., Weiner, B. J., Kartaltepe, J. S., Nakajima, K., Nayyeri, H., Stern, D., Kashikawa, N., & Spinrad, H. (2012). SPECTROSCOPIC CONFIRMATION OF THREE z-DROPOUT GALAXIES AT z=6.844-7.213: DEMOGRAPHICS OF Ly alpha EMISSION IN z similar to 7 GALAXIES. ASTROPHYSICAL JOURNAL, 744(2).
• Papovich, C., Bassett, R., Lotz, J. M., Wel, A., Tran, K., Finkelstein, S. L., Bell, E. F., Conselice, C. J., Dekel, A., Dunlop, J. S., Guo, Y., Faber, S. M., Farrah, D., Ferguson, H. C., Finkelstein, K. D., H "aussler, B., Kocevski, D. D., Koekemoer, A. M., Koo, D. C., , McGrath, E. J., et al. (2012). CANDELS Observations of the Structural Properties of Cluster Galaxies at z = 1.62. apj, 750, 93.
• Papovich, C., Bassett, R., Lotz, J. M., van, d., Tran, K. -., Finkelstein, S. L., Bell, E. F., Conselice, C. J., Dekel, A., Dunlop, J. S., Guo, Y., Faber, S. M., Farrah, D., Ferguson, H. C., Finkelstein, K. D., Haeussler, B., Kocevski, D. D., Koekemoer, A. M., Koo, D. C., , McGrath, E. J., et al. (2012). CANDELS OBSERVATIONS OF THE STRUCTURAL PROPERTIES OF CLUSTER GALAXIES AT z=1.62. ASTROPHYSICAL JOURNAL, 750(2).
• Rhoads, J. E., Hibon, P., Malhotra, S., Cooper, M., & Weiner, B. (2012). A Ly alpha GALAXY AT REDSHIFT z=6.944 IN THE COSMOS FIELD. ASTROPHYSICAL JOURNAL LETTERS, 752(2).
• Rhoads, J. E., Hibon, P., Malhotra, S., Cooper, M., & Weiner, B. (2012). A Ly$ alpha$ Galaxy at Redshift z = 6.944 in the COSMOS Field. apjl, 752, L28.
• Rhoads, J. E., Hibon, P., Malhotra, S., Cooper, M., & Weiner, B. (2012). A Lyman Alpha Galaxy at Redshift z=6.944 in the COSMOS Field.
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  Lyman-alpha emitting galaxies can be used to study cosmological reionization,because a neutral intergalactic medium scatters Lyman-alpha photons intodiffuse halos whose surface brightness falls below typical survey detectionlimits. Here we present the Lyman-alpha emitting galaxy LAEJ095950.99+021219.1, identified at redshift z=6.944 in the COSMOS field usingnarrowband imaging and followup spectroscopy with the IMACS instrument on theMagellan I Baade telescope. With a single object spectroscopically confirmed sofar, our survey remains consistent with a wide range of IGM neutral fraction atredshift seven, but further observations are planned and will help clarify thesituation. Meantime, the object we present here is only the third Lyman-alphaselected galaxy to be spectroscopically confirmed at redshift seven, and is2--3 times fainter than the previously confirmed redshift seven Lyman alphagalaxies.[Journal_ref: ]
• Rodney, S. A., Riess, A. G., Dahlen, T., Strolger, L., Ferguson, H. C., Hjorth, J., Frederiksen, T. F., Weiner, B. J., Mobasher, B., Casertano, S., Jones, D. O., Challis, P., Faber, S. M., Filippenko, A. V., Garnavich, P., Graur, O. r., Grogin, N. A., Hayden, B., Jha, S. W., , Kirshner, R. P., et al. (2012). A TYPE Ia SUPERNOVA AT REDSHIFT 1.55 IN HUBBLE SPACE TELESCOPE INFRARED OBSERVATIONS FROM CANDELS. ASTROPHYSICAL JOURNAL, 746(1).
• Rodney, S. A., Riess, A. G., Dahlen, T., Strolger, L., Ferguson, H. C., Hjorth, J., Frederiksen, T. F., Weiner, B. J., Mobasher, B., Casertano, S., Jones, D. O., Challis, P., Faber, S. M., Filippenko, A. V., Garnavich, P., Graur, O., Grogin, N. A., Hayden, B., Jha, S. W., , Kirshner, R. P., et al. (2012). A Type Ia Supernova at Redshift 1.55 in Hubble Space Telescope Infrared Observations from CANDELS. apj, 746, 5.
• Rujopakarn, W., Rieke, G. H., Papovich, C. J., Weiner, B. J., Rigby, J. R., Rex, M., Bian, F., Kuhn, O. P., & Thompson, D. (2012). Large Binocular Telescope and Spitzer Spectroscopy of Star-forming Galaxies at 1 ltz lt 3: Extinction and Star Formation Rate Indicators. apj, 755, 168.
• Sheth, K., Melbourne, J., Elmegreen, D. M., Elmegreen, B. G., Athanassoula, E., Abraham, R. G., & Weiner, B. J. (2012). HOT DISKS AND DELAYED BAR FORMATION. ASTROPHYSICAL JOURNAL, 758(2).
• Sheth, K., Melbourne, J., Elmegreen, D. M., Elmegreen, B. G., Athanassoula, E., Abraham, R. G., & Weiner, B. J. (2012). Hot Disks and Delayed Bar Formation. apj, 758, 136.
• Smith, N., Silverman, J. M., Filippenko, A. V., Cooper, M. C., Matheson, T., Bian, F., Weiner, B. J., & Comerford, J. M. (2012). SYSTEMATIC BLUESHIFT OF LINE PROFILES IN THE TYPE IIn SUPERNOVA 2010jl: EVIDENCE FOR POST-SHOCK DUST FORMATION?. ASTRONOMICAL JOURNAL, 143(1).
• Smith, N., Silverman, J. M., Filippenko, A. V., Cooper, M. C., Matheson, T., Bian, F., Weiner, B. J., & Comerford, J. M. (2012). Systematic Blueshift of Line Profiles in the Type IIn Supernova 2010jl: Evidence for Post-shock Dust Formation?. aj, 143, 17.
• Twite, J. W., Conselice, C. J., Buitrago, F., Noeske, K., Weiner, B. J., Acosta-Pulido, J. A., & Bauer, A. E. (2012). H$ alpha$ star formation rates in massive galaxies at z tilde 1. mnras, 420, 1061-1078.
• Twite, J. W., Conselice, C. J., Buitrago, F., Noeske, K., Weiner, B. J., Acosta-Pulido, J. A., & Bauer, A. E. (2012). Ha star formation rates in massive galaxies at z similar to 1. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 420(2), 1061-1078.
• Wang, T., Huang, J., Faber, S. M., Fang, G., Wuyts, S., Fazio, G. G., Yan, H., Dekel, A., Guo, Y., Ferguson, H. C., Grogin, N., Lotz, J. M., Weiner, B., McGrath, E. J., Kocevski, D., Hathi, N. P., Lucas, R. A., Koekemoer, A. M., Kong, X. u., & Gu, Q. (2012). CANDELS: CORRELATIONS OF SPECTRAL ENERGY DISTRIBUTIONS AND MORPHOLOGIES WITH STAR FORMATION STATUS FOR MASSIVE GALAXIES AT z similar to 2. ASTROPHYSICAL JOURNAL, 752(2).
• Wang, T., Huang, J., Faber, S. M., Fang, G., Wuyts, S., Fazio, G. G., Yan, H., Dekel, A., Guo, Y., Ferguson, H. C., Grogin, N., Lotz, J. M., Weiner, B., McGrath, E. J., Kocevski, D., Hathi, N. P., Lucas, R. A., Koekemoer, A. M., Kong, X., & Gu, Q. (2012). CANDELS: Correlations of Spectral Energy Distributions and Morphologies with Star formation Status for Massive Galaxies at z ~ 2. apj, 752, 134.
• Wu, J., Tsai, C., Sayers, J., Benford, D., Bridge, C., Blain, A., Eisenhardt, P. R., Stern, D., Petty, S., Assef, R., Bussmann, S., Comerford, J. M., Cutri, R., Evans, N. J., Griffith, R., Jarrett, T., Lake, S., Lonsdale, C., Rho, J., , Stanford, S. A., et al. (2012). Submillimeter Follow-up of WISE-selected Hyperluminous Galaxies. apj, 756, 96.
• Wu, J., Tsai, C., Sayers, J., Benford, D., Bridge, C., Blain, A., Eisenhardt, P., Stern, D., Petty, S., Assef, R., Bussmann, S., Comerford, J. M., Cutri, R., Evans, N., Griffith, R., Jarrett, T., Lake, S., Lonsdale, C., Rho, J., , Stanford, S. A., et al. (2012). SUBMILLIMETER FOLLOW-UP OF WISE-SELECTED HYPERLUMINOUS GALAXIES. ASTROPHYSICAL JOURNAL, 756(1).
• Wuyts, S., Schreiber, N. M., Genzel, R., Guo, Y., Barro, G., Bell, E. F., Dekel, A., Faber, S. M., Ferguson, H. C., Giavalisco, M., Grogin, N. A., Hathi, N. P., Huang, K., Kocevski, D. D., Koekemoer, A. M., Koo, D. C., Lotz, J., Lutz, D., McGrath, E., , Newman, J. A., et al. (2012). Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies. apj, 753, 114.
• Wuyts, S., Schreiber, N., Genzel, R., Guo, Y., Barro, G., Bell, E. F., Dekel, A., Faber, S. M., Ferguson, H. C., Giavalisco, M., Grogin, N. A., Hathi, N. P., Huang, K., Kocevski, D. D., Koekemoer, A. M., Koo, D. C., Lotz, J., Lutz, D., McGrath, E., , Newman, J. A., et al. (2012). SMOOTH(ER) STELLAR MASS MAPS IN CANDELS: CONSTRAINTS ON THE LONGEVITY OF CLUMPS IN HIGH-REDSHIFT STAR-FORMING GALAXIES. ASTROPHYSICAL JOURNAL, 753(2).
• Yan, H., Finkelstein, S. L., Huang, K., Ryan, R. E., Ferguson, H. C., Koekemoer, A. M., Grogin, N. A., Dickinson, M., Newman, J. A., Somerville, R. S., Dav 'e, R., Faber, S. M., Papovich, C., Guo, Y., Giavalisco, M., Lee, K., Reddy, N., Cooray, A. R., Siana, B. D., , Hathi, N. P., et al. (2012). Luminous and High Stellar Mass Candidate Galaxies at z ap 8 Discovered in the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey. apj, 761, 177.
• Yan, H., Finkelstein, S. L., Huang, K., Ryan, R. E., Ferguson, H. C., Koekemoer, A. M., Grogin, N. A., Dickinson, M., Newman, J. A., Somerville, R. S., Dave, R., Faber, S. M., Papovich, C., Guo, Y., Giavalisco, M., Lee, K., Reddy, N., Cooray, A. R., Siana, B. D., , Hathi, N. P., et al. (2012). LUMINOUS AND HIGH STELLAR MASS CANDIDATE GALAXIES AT z approximate to 8 DISCOVERED IN THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY. ASTROPHYSICAL JOURNAL, 761(2).
• Coil, A. L., Weiner, B. J., Holz, D. E., Cooper, M. C., Yan, R., & Aird, J. (2011). OUTFLOWING GALACTIC WINDS IN POST-STARBURST AND ACTIVE GALACTIC NUCLEUS HOST GALAXIES AT 0.2 < z < 0.8. ASTROPHYSICAL JOURNAL, 743(1).
• Dutton, A. A., van, d., Faber, S. M., Simard, L., Kassin, S. A., Koo, D. C., Bundy, K., Huang, J., Weiner, B. J., Cooper, M. C., Newman, J. A., Mozena, M., & Koekemoer, A. M. (2011). On the evolution of the velocity-mass-size relations of disc-dominated galaxies over the past 10 billion years. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 410(3), 1660-1676.
• Grogin, N. A., Kocevski, D. D., Faber, S. M., Ferguson, H. C., Koekemoer, A. M., Riess, A. G., Acquaviva, V., Alexander, D. M., Almaini, O., Ashby, M., Barden, M., Bell, E. F., Bournaud, F., Brown, T. M., Caputi, K. I., Casertano, S., Cassata, P., Castellano, M., Challis, P., , Chary, R., et al. (2011). CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 197(2).
• Kassin, S. A., Fogarty, L., Goodsall, T., Clarke, F. J., Houghton, R., Salter, G., Thatte, N., Tecza, M., Davies, R. L., Weiner, B. J., Willmer, C., Salim, S., Cooper, M. C., Newman, J. A., Bundy, K., Conselice, C. J., Koekemoer, A. M., Lin, L., Moustakas, L. A., & Wang, T. (2011). Oxford SWIFT integral field spectrograph and multiwavelength observations of the Eagle galaxy at z=0.77. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 417(4), 2882-2890.
• Koekemoer, A. M., Faber, S. M., Ferguson, H. C., Grogin, N. A., Kocevski, D. D., Koo, D. C., Lai, K., Lotz, J. M., Lucas, R. A., McGrath, E. J., Ogaz, S., Rajan, A., Riess, A. G., Rodney, S. A., Strolger, L., Casertano, S., Castellano, M., Dahlen, T., Dickinson, M., , Dolch, T., et al. (2011). CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY-THE HUBBLE SPACE TELESCOPE OBSERVATIONS, IMAGING DATA PRODUCTS, AND MOSAICS. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 197(2).
• Prochaska, J. X., Weiner, B., Chen, H. -., Mulchaey, J., & Cooksey, K. (2011). PROBING THE INTERGALACTIC MEDIUM/GALAXY CONNECTION. V. ON THE ORIGIN OF Ly alpha AND O VI ABSORPTION AT z < 0.2. ASTROPHYSICAL JOURNAL, 740(2).
• Trump, J. R., Weiner, B. J., Scarlata, C., Kocevski, D. D., Bell, E. F., McGrath, E. J., Koo, D. C., Faber, S. M., Laird, E. S., Mozena, M., Rangel, C., Yan, R., Yesuf, H., Atek, H., Dickinson, M., Donley, J. L., Dunlop, J. S., Ferguson, H. C., Finkelstein, S. L., , Grogin, N. A., et al. (2011). A CANDELS WFC3 GRISM STUDY OF EMISSION-LINE GALAXIES AT z similar to 2: A MIX OF NUCLEAR ACTIVITY AND LOW-METALLICITY STAR FORMATION. ASTROPHYSICAL JOURNAL, 743(2).
• Yan, R., Ho, L. C., Newman, J. A., Coil, A. L., Willmer, C., Laird, E. S., Georgakakis, A., Aird, J., Barmby, P., Bundy, K., Cooper, M. C., Davis, M., Faber, S. M., Fang, T., Griffith, R. L., Koekemoer, A. M., Koo, D. C., Nandra, K., Park, S. Q., , Sarajedini, V. L., et al. (2011). AEGIS: DEMOGRAPHICS OF X-RAY AND OPTICALLY SELECTED ACTIVE GALACTIC NUCLEI. ASTROPHYSICAL JOURNAL, 728(1).
• van, d., Straughn, A. N., Rix, H. -., Finkelstein, S. L., Koekemoer, A. M., Weiner, B. J., Wuyts, S., Bell, E. F., Faber, S. M., Trump, J. R., Koo, D. C., Ferguson, H. C., Scarlata, C., Hathi, N. P., Dunlop, J. S., Newman, J. A., Dickinson, M., Jahnke, K., Salmon, B. W., , de, M., et al. (2011). EXTREME EMISSION-LINE GALAXIES IN CANDELS: BROADBAND-SELECTED, STARBURSTING DWARF GALAXIES AT z > 1. ASTROPHYSICAL JOURNAL, 742(2).
• Chen, Y., Tremonti, C. A., Heckman, T. M., Kauffmann, G., Weiner, B. J., Brinchmann, J., & Wang, J. (2010). ABSORPTION-LINE PROBES OF THE PREVALENCE AND PROPERTIES OF OUTFLOWS IN PRESENT-DAY STAR-FORMING GALAXIES. ASTRONOMICAL JOURNAL, 140(2), 445-461.
• Chen, Y., Tremonti, C. A., Heckman, T. M., Kauffmann, G., Weiner, B. J., Brinchmann, J., & Wang, J. (2010). Absorption-line probes of the prevalence and properties of outflows in present-day star-forming galaxies. The Astronomical Journal, 445-461.
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  We analyze star forming galaxies drawn from SDSS DR7 to show how theinterstellar medium (ISM) Na I 5890, 5896 (Na D) absorption lines depend ongalaxy physical properties, and to look for evidence of galactic winds. Wecombine the spectra of galaxies with similar geometry/physical parameters tocreate composite spectra with signal-to-noise ~300. The stellar continuum ismodeled using stellar population synthesis models, and the continuum-normalizedspectrum is fit with two Na I absorption components. We find that: (1) ISM Na Dabsorption lines with equivalent widths EW > 0.8A are only prevalent in diskgalaxies with specific properties -- large extinction (Av), high star formationrates (SFR), high star formation rate per unit area ($\Sigma_{\rm SFR}$), orhigh stellar mass (M*). (2) the ISM Na D absorption lines can be separated intotwo components: a quiescent disk-like component at the galaxy systemic velocityand an outflow component; (3) the disk-like component is much stronger in theedge-on systems, and the outflow component covers a wide angle but is strongerwithin 60deg of the disk rotation axis; (4) the EW and covering factor of thedisk component correlate strongly with dust attenuation, highlighting theimportance that dust shielding may play the survival of Na I. (5) The EW of theoutflow component depends primarily on $\Sigma_{\rm SFR}$ and secondarily onAv; (6) the outflow velocity varies from ~120 to 160km/s but shows little hintof a correlation with galaxy physical properties over the modest dynamic rangethat our sample probes (1.2 dex in log$\Sigma_{\rm SFR}$ and 1 dex in log M*).[Journal_ref: The Astronomical Journal 140 (2010) 445-461]
• Cooper, M. C., Coil, A. L., Gerke, B. F., Newman, J. A., Bundy, K., Conselice, C. J., Croton, D. J., Davis, M., Faber, S. M., Guhathakurta, P., Koo, D. C., Lin, L., Weiner, B. J., Willmer, C., & Yan, R. (2010). Absence of evidence is not evidence of absence: the colour-density relation at fixed stellar mass persists to z similar to 1. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 409(1), 337-345.
• Covington, M. D., Kassin, S. A., Dutton, A. A., Weiner, B. J., Cox, T. J., Jonsson, P., Primack, J. R., Faber, S. M., & Koo, D. C. (2010). EVOLUTION OF THE STELLAR MASS TULLY-FISHER RELATION IN DISK GALAXY MERGER SIMULATIONS. ASTROPHYSICAL JOURNAL, 710(1), 279-288.
• Genzel, R., Tacconi, L. J., Gracia-Carpio, J., Sternberg, A., Cooper, M. C., Shapiro, K., Bolatto, A., Bouche, N., Bournaud, F., Burkert, A., Combes, F., Comerford, J., Cox, P., Davis, M., Schreiber, N., Garcia-Burillo, S., Lutz, D., Naab, T., Neri, R., , Omont, A., et al. (2010). A study of the gas-star formation relation over cosmic time. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 407(4), 2091-2108.
• Rubin, K., Prochaska, J. X., Koo, D. C., Phillips, A. C., & Weiner, B. J. (2010). GALAXIES PROBING GALAXIES: COOL HALO GAS FROM A z=0.47 POST-STARBURST GALAXY. ASTROPHYSICAL JOURNAL, 712(1), 574-584.
• Rubin, K., Weiner, B. J., Koo, D. C., Martin, C. L., Prochaska, J. X., Coil, A. L., & Newman, J. A. (2010). THE PERSISTENCE OF COOL GALACTIC WINDS IN HIGH STELLAR MASS GALAXIES BETWEEN z similar to 1.4 AND similar to 1*. ASTROPHYSICAL JOURNAL, 719(2), 1503-1525.
• Tacconi, L. J., Genzel, R., Neri, R., Cox, P., Cooper, M. C., Shapiro, K., Bolatto, A., Bouche, N., Bournaud, F., Burkert, A., Combes, F., Comerford, J., Davis, M., Schreiber, N., Garcia-Burillo, S., Gracia-Carpio, J., Lutz, D., Naab, T., Omont, A., , Shapley, A., et al. (2010). High molecular gas fractions in normal massive star-forming galaxies in the young Universe. NATURE, 463(7282), 781-784.
• Coil, A. L., Georgakakis, A., Newman, J. A., Cooper, M. C., Croton, D., Davis, M., Koo, D. C., Laird, E. S., Nandra, K., Weiner, B. J., Willmer, C., & Yan, R. (2009). AEGIS: THE CLUSTERING OF X-RAY ACTIVE GALACTIC NUCLEUS RELATIVE TO GALAXIES AT z similar to 1. ASTROPHYSICAL JOURNAL, 701(2), 1484-1499.
• Rieke, G. H., Alonso-Herrero, A., Weiner, B. J., Perez-Gonzalez, P. G., Blaylock, M., Donley, J. L., & Marcillac, D. (2009). DETERMINING STAR FORMATION RATES FOR INFRARED GALAXIES. ASTROPHYSICAL JOURNAL, 692(1), 556-573.
• Salim, S., Dickinson, M., Rich, R. M., Charlot, S., Lee, J. C., Schiminovich, D., Perez-Gonzalez, P. G., Ashby, M., Papovich, C., Faber, S. M., Ivison, R. J., Frayer, D. T., Walton, J. M., Weiner, B. J., Chary, R., Bundy, K., Noeske, K., & Koekemoer, A. M. (2009). MID-IR LUMINOSITIES AND UV/OPTICAL STAR FORMATION RATES AT z < 1.4. ASTROPHYSICAL JOURNAL, 700(1), 161-182.
• Weiner, B. J. (2009). Star Formation Driven Galactic Winds at z similar to 1.4. MONSTER'S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS, 1201, 142-145.
• Weiner, B. J., Coil, A. L., Prochaska, J. X., Newman, J. A., Cooper, M. C., Bundy, K., Conselice, C. J., Dutton, A. A., Faber, S. M., Koo, D. C., Lotz, J. M., Rieke, G. H., & Rubin, K. (2009). UBIQUITOUS OUTFLOWS IN DEEP2 SPECTRA OF STAR-FORMING GALAXIES AT z=1.4. ASTROPHYSICAL JOURNAL, 692(1), 187-211.
• Yan, R., Newman, J. A., Faber, S. M., Coil, A. L., Cooper, M. C., Davis, M., Weiner, B. J., Gerke, B. F., & Koo, D. C. (2009). The DEEP2 Galaxy Redshift Survey: environments of post-starburst galaxies at z similar to 0.1 and similar to 0.8. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 398(2), 735-753.
• Coil, A. L., Newman, J. A., Croton, D., Cooper, M. C., Davis, M., Faber, S. M., Gerke, B. F., Koo, D. C., Padmanabhan, N., Wechsler, R. H., & Weiner, B. J. (2008). The DEEP2 Galaxy Redshift Survey: Color and luminosity dependence of galaxy clustering at z similar to 1. ASTROPHYSICAL JOURNAL, 672(1), 153-176.
• Cooksey, K. L., Prochaska, J. X., Chen, H., Mulchaey, J. S., & Weiner, B. J. (2008). Characterizing the low-redshift intergalactic medium toward PKS 1302-102. ASTROPHYSICAL JOURNAL, 676(1), 262-285.
• Cooper, M. C., Newman, J. A., Weiner, B. J., Yan, R., Willmer, C., Bundy, K., Coil, A. L., Conselice, C. J., Davis, M., Faber, S. M., Gerke, B. F., Guhathakurta, P., Koo, D. C., & Noeske, K. G. (2008). The DEEP2 Galaxy Redshift Survey: the role of galaxy environment in the cosmic star formation history. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 383(3), 1058-1078.
• Lin, L., Patton, D. R., Koo, D. C., Casteels, K., Conselice, C. J., Faber, S. M., Lotz, J., Willmer, C., Hsieh, B. C., Chiueh, T., Newman, J. A., Novak, G. S., Weiner, B. J., & Cooper, M. C. (2008). The redshift evolution of wet, dry, and mixed galaxy mergers from close galaxy pairs in the DEEP2 galaxy Redshift Survey. ASTROPHYSICAL JOURNAL, 681(1), 232-243.
• Lotz, J. M., Davis, M., Faber, S. M., Guhathakurta, P., Gwyn, S., Huang, J., Koo, D. C., Le, F. E., Lin, L., Newman, J., Noeske, K., Papovich, C., Willmer, C., Coil, A., Conselice, C. J., Cooper, M., Hopkins, A. M., Metevier, A., Primack, J., , Rieke, G., et al. (2008). The evolution of galaxy mergers and morphology at z < 1.2 in the Extended Groth Strip. ASTROPHYSICAL JOURNAL, 672(1), 177-197.
• Sawicki, M., Lemaux, B. C., Guhathakurta, P., Kirby, E. N., Konidaris, N. P., Martin, C. L., Cooper, M. C., Koo, D. C., Newman, J. A., & Weiner, B. J. (2008). THE DEEP2 REDSHIFT SURVEY: Ly alpha EMITTERS IN THE SPECTROSCOPIC DATABASE. ASTROPHYSICAL JOURNAL, 687(2), 884-898.
• Conselice, C. J., Bundy, K., Trujillo, I., Coil, A., Eisenhardt, P., Ellis, R. S., Georgakakis, A., Huang, J., Lotz, J., Nandra, K., Newman, J., Papovich, C., Weiner, B., & Willmer, C. (2007). The properties and evolution of a K-band selected sample of massive galaxies at z similar to 0.4-2 in the Palomar/DEEP2 survey. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 381(3), 962-986.
• Cooper, M. C., Newman, J. A., Coil, A. L., Croton, D. J., Gerke, B. F., Yan, R., Davis, M., Faber, S. M., Guhathakurta, P., Koo, D. C., Weiner, B. J., & Willmer, C. (2007). The DEEP2 galaxy redshift survey: evolution of the colour-density relation at 0.4 < z < 1.35. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 376(4), 1445-1459.
• Davis, M., Guhathakurta, P., Konidaris, N. P., Newman, J. A., Ashby, M., Biggs, A. D., Barmby, P., Bundy, K., Chapman, S. C., Coil, A. L., Conselice, C. J., Cooper, M. C., Croton, D. J., Eisenhardt, P., Ellis, R. S., Faber, S. M., Fang, T., Fazio, G. G., Georgakakis, A., , Gerke, B. F., et al. (2007). The All-Wavelength Extended Groth Strip International Survey (AEGIS) data sets. ASTROPHYSICAL JOURNAL, 660(1), L1-L6.
• Faber, S. M., Willmer, C., Wolf, C., Koo, D. C., Weiner, B. J., Newman, J. A., Im, M., Coil, A. L., Conroy, C., Cooper, M. C., Davis, M., Finkbeiner, D. P., Gerke, B. F., Gebhardt, K., Groth, E. J., Guhathakurta, P., Harker, J., Kaiser, N., Kassin, S., , Kleinheinrich, M., et al. (2007). Galaxy luminosity functions to z similar to 1 from deep2 and combo-17: Implications for red galaxy formation. ASTROPHYSICAL JOURNAL, 665(1), 265-294.
• Gerke, B. F., Newman, J. A., Faber, S. M., Cooper, M. C., Croton, D. J., Davis, M., Willmer, C., Yan, R., Coil, A. L., Guhathakurta, P., Koo, D. C., & Weiner, B. J. (2007). The DEEP2 galaxy redshift survey: the evolution of the blue fraction in groups and the field. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 376(4), 1425-1444.
• Gerke, B. F., Newman, J. A., Lotz, J., Yan, R., Barmby, P., Coil, A. L., Conselice, C. J., Ivison, R. J., Lin, L., Koo, D. C., Nandra, K., Salim, S., Small, T., Weiner, B. J., Cooper, M. C., Davis, M., Faber, S. M., & Guhathakurta, P. (2007). The DEEP2 Galaxy Redshift Survey: AEGIS observations of a dual AGN at z=0.7. ASTROPHYSICAL JOURNAL, 660(1), L23-L26.
• Kassin, S. A., Weiner, B. J., Faber, S. M., Koo, D. C., & Lotz, J. M. (2007). The stellar mass tully-fisher relation to z=1.2. AT THE EDGE OF THE UNIVERSE: LATEST RESULTS FROM THE DEEPEST ASTRONOMICAL SURVEYS, 380, 477-482.
• Kassin, S. A., Weiner, B. J., Faber, S. M., Koo, D. C., Lotz, J. M., Diemand, J., Harker, J. J., Bundy, K., Metevier, A. J., Phillips, A. C., Cooper, M. C., Croton, D. J., Konidaris, N., Noeske, K. G., & Willmer, C. (2007). The stellar mass Tully-Fisher relation to z=1.2 from AEGIS. ASTROPHYSICAL JOURNAL, 660(1), L35-L38.
• Kirby, E. N., Guhathakurta, P., Faber, S. M., Koo, D. C., Weiner, B. J., & Cooper, M. C. (2007). The deep2 galaxy redshift survey: Redshift identification of single-line emission galaxies. ASTROPHYSICAL JOURNAL, 660(1), 62-71.
• Lin, L., Koo, D. C., Weiner, B. J., Chiueh, T., Coil, A. L., Lotz, J., Conselice, C. J., Willner, S. P., Smith, H. A., Guhathakurta, P., Huang, J., Le, F. E., Noeske, K. G., Willmer, C., Cooper, M. C., & Phillips, A. C. (2007). AEGIS: Enhancement of dust-enshrouded star formation in close galaxy pairs and merging galaxies up to z similar to 1. ASTROPHYSICAL JOURNAL, 660(1), L51-L54.
• Noeske, K. G., Faber, S. M., Weiner, B. J., Koo, D. C., Primack, J. R., Dekel, A., Papovich, C., Conselice, C. J., Le, F. E., Rieke, G. H., Coil, A. L., Lotz, J. M., Somerville, R. S., & Bundy, K. (2007). Star formation in AEGIS field galaxies since z=1.1: Staged galaxy formation and a model of mass-dependent gas exhaustion. ASTROPHYSICAL JOURNAL, 660(1), L47-L50.
• Noeske, K. G., Weiner, B. J., Faber, S. M., Papovich, C., Koo, D. C., Somerville, R. S., Bundy, K., Conselice, C. J., Newman, J. A., Schiminovich, D., Le, F. E., Coil, A. L., Rieke, G. H., Lotz, J. M., Primack, J. R., Barmby, P., Cooper, M. C., Davis, M., Ellis, R. S., , Fazio, G. G., et al. (2007). Star formation in AEGIS field galaxies since z=1.1: The dominance of gradually declining star formation, and the main sequence of star-forming galaxies. ASTROPHYSICAL JOURNAL, 660(1), L43-L46.
• Pierce, C. M., Lotz, J. M., Laird, E. S., Lin, L., Nandra, K., Primack, J. R., Faber, S. M., Barmby, P., Park, S. Q., Willner, S. P., Gwyn, S., Koo, D. C., Coil, A. L., Cooper, M. C., Georgakakis, A., Koekemoer, A. M., Noeske, K. G., Weiner, B. J., & Willmer, C. (2007). Aegis: Host galaxy morphologies of X-ray-selected and infrared-selected active galactic nuclei at 0.2 <= z < 1.2. ASTROPHYSICAL JOURNAL, 660(1), L19-L22.
• Weiner, B. J., Papovich, C., Bundy, K., Conselice, C. J., Cooper, M. C., Ellis, R. S., Ivison, R. J., Noeske, K. G., Phillips, A. C., & Yan, R. (2007). AEGIS: Extinction and Star Formation Tracers from Line Emission. Astrophys.J., 660.
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  Strong nebular emission lines are a sensitive probe of star formation andextinction in galaxies, and the [O II] line detects star forming populationsout to z>1. However, star formation rates from emission lines depend oncalibration of extinction and the [O II]/H-alpha line ratio, and separatingstar formation from AGN emission. We use calibrated line luminosities from theDEEP2 survey and Palomar K magnitudes to show that the behavior of emissionline ratios depends on galaxy magnitude and color. For galaxies on the blueside of the color bimodality, the vast majority show emission signatures ofstar formation, and there are strong correlations of extinction and [OII]/H-alpha with restframe H magnitude. The conversion of [O II] toextinction-corrected H-alpha and thus to star formation rate has a significantslope with M_H, 0.23 dex/mag. Red galaxies with emission lines have a muchhigher scatter in their line ratios, and more than half show AGN signatures. Weuse 24 micron fluxes from Spitzer/MIPS to demonstrate the differing populationsprobed by nebular emission and by mid-IR luminosity. Although extinction iscorrelated with luminosity, 98% of IR-luminous galaxies at z~1 are stilldetected in the [O II] line. Mid-IR detected galaxies are mostly bright andintermediate color, while fainter, bluer galaxies with high [O II] luminosityare rarely detected at 24 microns.[Journal_ref: Astrophys.J.660:L39-L42,2007]
• Weiner, B. J., Papovich, C., Bundy, K., Conselice, C. J., Cooper, M. C., Ellis, R. S., Ivison, R. J., Noeske, K. G., Phillips, A. C., & Yan, R. (2007). AEGIS: Extinction and star formation tracers from line emission. ASTROPHYSICAL JOURNAL, 660(1), L39-L42.
• Bundy, K., Ellis, R. S., Conselice, C. J., Taylor, J. E., Cooper, M. C., Willmer, C., Weiner, B. J., Coil, A. L., Noeske, K. G., & Eisenhardt, P. (2006). The mass assembly history of field galaxies: Detection of an evolving mass limit for starforming galaxies. ASTROPHYSICAL JOURNAL, 651(1), 120-141.
• Cooper, M. C., Newman, J. A., Croton, D. J., Weiner, B. J., Willmer, C., Gerke, B. F., Madgwick, D. S., Faber, S. M., Davis, M., Coil, A. L., Finkbeiner, D. P., Guhathakurta, P., & Koo, D. C. (2006). The DEEP2 Galaxy Redshift Survey: the relationship between galaxy properties and environment at z similar to 1. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 370(1), 198-212.
• Harker, J. J., Schiavon, R. P., Weiner, B. J., & Faber, S. M. (2006). Population Synthesis Models for Late Build-Up of the Red Sequence. Astrophys.J., 647.
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  We present population synthesis models designed to represent the starformation histories of L* red sequence galaxies (RSGs). Earlier work has shownthat single-burst stellar populations (SSPs) are unable to match Balmer linestrengths simultaneously at high and low redshift. We therefore consideralternative star formation histories in which RSGs contain intermediate-agedstars even at late epochs. The models are compared to Balmer Hdelta absorptionstrengths, U-B color data, and the number density of red sequence galaxies fromz=1 to z=0. We find that quenched models (which consist of constant starformation histories truncated at regularly-spaced intervals) average to an RSGpopulation that matches the data well, showing slow evolution in color andBalmer line strength and a rise in number density by a factor of a few afterz=1. The data are best fit by a turn-on of quenching at redshifts z=1.5-2.[Journal_ref: Astrophys.J.647:L103-L106,2006]
• Harker, J. J., Schiavon, R. P., Weiner, B. J., & Faber, S. M. (2006). Population synthesis models for late buildup of the red sequence. ASTROPHYSICAL JOURNAL, 647(2), L103-L106.
• Kassin, S. A., de Jong, R. S., & Weiner, B. J. (2006). Dark and Baryonic Matter in Bright Spiral Galaxies: II. Radial Distributions for 34 Galaxies. Astrophys.J., 804-824.
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  We decompose the rotation curves of 34 bright spiral galaxies into baryonicand dark matter components. Stellar mass profiles are created by applyingcolor-M/L relations to near-infrared and optical photometry. We find that theradial profile of the baryonic-to-dark-matter ratio is self-similar for allgalaxies, when scaled to the radius where the contribution of the baryonic massto the rotation curve equals that of the dark matter (R_X). We argue that thisis due to the quasi-exponential nature of disks and rotation curves that arenearly flat after an initial rise. The radius R_X is found to correlate moststrongly with baryonic rotation speed, such that galaxies with R_X measurementsthat lie further out in their disks rotate faster. This quantity alsocorrelates very strongly with stellar mass, Hubble type, and observed rotationspeed; B-band central surface brightness is less related to R_X than theseother galaxy properties. Most of the galaxies in our sample appear to be closeto maximal disk. For these galaxies, we find that maximum observed rotationspeeds are tightly correlated with maximum rotation speeds predicted from thebaryon distributions, such that one can create a Tully-Fisher relation based onsurface photometry and redshifts alone. Finally, we compare our data to the NFWparameterization for dark matter profiles with and without including adiabaticcontraction as it is most commonly implemented. Fits are generally poor, andall but 2 galaxies are better fit if adiabatic contraction is not performed. Inorder to have better fits, and especially to accommodate adiabatic contraction,baryons would need to contribute very little to the total mass in the innerparts of galaxies, seemingly in contrast with other observational constraints.[Journal_ref: Astrophys.J. 643 (2006) 804-824]
• Prochaska, J. X., Weiner, B. J., Chen, H., & Mulchaey, J. S. (2006). Probing the intergalactic medium-galaxy connection toward PKS 0405-123. III. The galaxy survey and correlations with OVI absorbers. ASTROPHYSICAL JOURNAL, 643(2), 680-691.
• Schiavon, R. P., Faber, S. M., Konidaris, N., Graves, G., Willmer, C., Weiner, B. J., Coil, A. L., Cooper, M. C., Davis, M., Harker, J., Koo, D. C., Newman, J. A., & Yan, R. (2006). The DEEP2 galaxy redshift survey: Mean ages and metallicities of red field galaxies at z similar to 0.9 from stacked Keck DEIMOS spectra. ASTROPHYSICAL JOURNAL, 651(2), L93-L96.
• Weiner, B. J., Willmer, C. N., Faber, S. M., Harker, J., Kassin, S. A., Phillips, A. C., Melbourne, J., Metevier, A. J., Vogt, N. P., & Koo, D. C. (2006). A Survey of Galaxy Kinematics to z ~ 1 in the TKRS/GOODS-N Field. II. Evolution in the Tully-Fisher Relation. Astrophys.J., 653, 1049-1069.
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  We use kinematic measurements of a large sample of galaxies from the TeamKeck Redshift Survey in the GOODS-N field to measure evolution in the opticaland near-IR Tully-Fisher relations to z = 1.2. We construct Tully-Fisherrelations with integrated line-of-sight velocity widths of ~ 1000 galaxies in Band ~ 670 in J-band; these relations have large scatter, and we derive amaximum-likelihood least squares method for fitting in the presence of scatter.The B-band Tully-Fisher relations, from z=0.4 to z=1.2, show evolution of ~1.0-1.5 mag internal to our sample without requiring calibration to a local TFrelation. There is evolution in both Tully-Fisher intercept and slope,suggesting differential luminosity evolution. In J-band, there is evolution inslope but little evolution in overall luminosity. The slope measurements implythat bright, massive blue galaxies fade {\it more strongly} than fainter bluegalaxies from z ~ 1.2 to now. This conclusion runs counter to some previousmeasurements and to our naive expectations, but we present a simple set of starformation histories to show that it arises naturally if massive galaxies haveshorter timescales of star formation, forming most of their stars before z ~ 1,while less massive galaxies form stars at more slowly declining rates. Thismodel predicts that the higher global star formation rate at z ~ 1 is mostlydue to higher SFR in massive galaxies. The amount of fading in B-bandconstrains star formation timescale more strongly than redshift of formation.Tully-Fisher and color-magnitude relations can provide global constraints onthe luminosity evolution and star formation history of blue galaxies.[Journal_ref: Astrophys.J.653:1049-1069,2006]
• Weiner, B. J., Willmer, C. N., Faber, S. M., Melbourne, J., Kassin, S. A., Phillips, A. C., Harker, J., Metevier, A. J., Vogt, N. P., & Koo, D. C. (2006). A Survey of Galaxy Kinematics to z ~ 1 in the TKRS/GOODS-N Field. I. Rotation and Dispersion Properties. Astrophys.J., 653, 1027-1048.
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  We present kinematic measurements of a large sample of galaxies from the TKRSSurvey in the GOODS-N field. We measure line-of-sight velocity dispersions fromintegrated emission for 1089 galaxies with median z=0.637, and spatiallyresolved kinematics for a subsample of 380 galaxies. This is the largest sampleof galaxies to z ~ 1 with kinematics to date, and allows us to measurekinematic properties without morphological pre-selection. Emission linewidthsprovide kinematics for the bulk of blue galaxies. To fit the spatially resolvedkinematics, we fit models with both line-of-sight rotation amplitude andvelocity dispersion. Integrated linewidth correlates well with a combination ofthe rotation gradient and dispersion, and is a robust measure of galaxykinematics. The spatial extents of emission and continuum are similar and thereis no evidence that linewidths are affected by nuclear or clumpy emission. Themeasured rotation gradient depends strongly on slit PA alignment with galaxymajor axis, but integrated linewidth does not. Even for galaxies withwell-aligned slits, some have kinematics dominated by dispersion (V/sigma
• Weiner, B. J., Willmer, C., Faber, S. M., Harker, J., Kassin, S. A., Phillips, A. C., Melbourne, J., Metevier, A. J., Vogt, N. P., & Koo, D. C. (2006). A survey of galaxy kinematics to z similar to 1 in the TKRS/GOODS-N field. II. Evolution in the Tully-Fisher relation. ASTROPHYSICAL JOURNAL, 653(2), 1049-1069.
• Weiner, B. J., Willmer, C., Faber, S. M., Melbourne, J., Kassin, S. A., Phillips, A. C., Harker, J., Metevier, A. J., Vogt, N. P., & Koo, D. C. (2006). A survey of galaxy kinematics to z similar to 1 in the TKRS/GOODS-N field. I. Rotation and dispersion properties. ASTROPHYSICAL JOURNAL, 653(2), 1027-1048.
• Willmer, C., Faber, S. M., Koo, D. C., Weiner, B. J., Newman, J. A., Coil, A. L., Connolly, A. J., Conroy, C., Cooper, M. C., Davis, M., Finkbeiner, D. P., Gerke, B. F., Guhathakurta, P., Harker, J., Kaiser, N., Kassin, S., Konidaris, N. P., Lin, L., Luppino, G., , Madgwick, D. S., et al. (2006). The deep evolutionary exploratory probe 2 galaxy redshift survey: The galaxy luminosity function to z similar to 1. ASTROPHYSICAL JOURNAL, 647(2), 853-873.
• Davis, M., Faber, S. M., Newman, J. A., Phillips, A. C., Ellis, R. S., Steidel, C. C., Conselice, C., Coil, A. L., Finkbeiner, D. P., Koo, D. C., Guhathakurta, P., Weiner, B., Schiavon, R., Willmer, C., Kaiser, N., Luppino, G., Wirth, G., Connolly, A., Eisenhardt, P., , Cooper, M., et al. (2003). Science objectives and early results of the DEEP2 Redshift Survey. DISCOVERIES AND RESEARCH PROSPECTS FROM 6- TO 10- METER-CLASS TELESCOPES II, 4834, 161-172.
• Gebhardt, K., Faber, S. M., Koo, D. C., Im, M., Simard, L., Illingworth, G. D., Phillips, A. C., Sarajedini, V. L., Vogt, N. P., Weiner, B., & Willmer, C. (2003). The deep Groth Strip survey. IX. Evolution of the fundamental plane of field galaxies. ASTROPHYSICAL JOURNAL, 597(1), 239-262.
• Weiner, B. J., Sellwood, J. A., & Williams, T. B. (2001). The Disk and Dark Halo Mass of the Barred Galaxy NGC 4123. II. Fluid-Dynamical Models. Astrophys.J., 546, 931-951.
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  We report a dynamical determination of the separate contributions of disk anddark halo masses to the rotation curve of a spiral galaxy. We usefluid-dynamical models of gas flow in the barred galaxy NGC 4123 to constrainthe dynamical properties of the galaxy: disk M/L, bar pattern speed, and thecentral density and scale radius of the dark halo. We derive a realistic barredpotential directly from the light distribution. For each model we assume avalue of the stellar M/L and a bar pattern speed Omega_p and add a dark halo tofit the rotation curve. We then compute the gas flow velocities with a 2-D gasdynamical code, and compare the model flow patterns to a 2-D velocity fieldderived from Fabry-Perot observations. The strong shocks and non-circularmotions in the observed gas flow require a high stellar M/L and a fast-rotatingbar. Models with I-band disk M/L of 2.0 -- 2.5 h_75, or 80 -- 100% of themaximum disk value, are highly favored. The corotation radius of the bar mustbe
• Weiner, B. J., Williams, T. B., Gorkom, V. J., & Sellwood, J. A. (2001). The Disk and Dark Halo Mass of the Barred Galaxy NGC 4123. I. Observations. Astrophys.J., 546, 916-930.
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  The non-circular streaming motions in barred galaxies are sensitive to themass of the bar and can be used to lift the degeneracy between disk and darkmatter halo encountered when fitting axisymmetric rotation curves of diskgalaxies. In this paper, we present photometric and kinematic observations ofNGC 4123, a barred galaxy of modest size (V_rot = 130 km/sec, L = 0.7 L_*),which reveal strong non-circular motions. The bar has straight dust lanes andan inner Lindblad resonance. The disk of NGC 4123 has no sign of truncation outto 10 scale lengths, and star-forming regions are found well outside R_25. AFabry-Perot H-alpha velocity field shows velocity jumps of >100 km/sec at thelocation of the dust lanes within the bar, indicating shocks in the gas flow.VLA observations yield the velocity field of the H I disk. Axisymmetric massmodels yield good fits to the rotation curve outside the bar regionfor diskI-band M/L of 2.25 or less, and dark halos with either isothermal or power-lawprofiles can fit the data well. In a companion paper, we model the full 2-Dvelocity field, including non-circular motions, to determine the stellar M/Land the mass of the dark halo.[Journal_ref: Astrophys.J.546:916-930,2001]
• Weiner, B. J., & Sellwood, J. A. (1999). The properties of the Galactic bar implied by gas kinematics in the inner Milky Way. Astrophys.J., 524, 112-128.
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  Longitude-velocity (l-V) diagrams of H I and CO gas in the inner Milky Wayhave long been known to be inconsistent with circular motion in an axisymmetricpotential. Several lines of evidence suggest that the Galaxy is barred, and gasflow in a barred potential could be consistent with the observed ``forbidden''velocities and other features in the data. We compare the H I observations tol-V diagrams synthesized from 2-D fluid dynamical simulations of gas flows in afamily of barred potentials. The gas flow pattern is very sensitive to theparameters of the assumed potential, which allows us to discriminate amongmodels. We present a model that reproduces the outer contour of the H I l-Vdiagram reasonably well; this model has a strong bar with a semimajor axis of3.6 kpc, an axis ratio of approximately 3:1, an inner Lindblad resonance (ILR),and a pattern speed of 42 km/s/kpc, and matches the data best when viewed from34\deg to the bar major axis. The behavior of the models, combined with theconstraint that the shocks in the Milky Way bar should resemble those inexternal barred galaxies, leads us to conclude that wide ranges of parameterspace are incompatible with the observations. In particular we suggest that thebar must be fairly strong, must have an ILR, and cannot be too end-on, with thebar major axis at 35\deg +/- 5\deg to the line of sight. The H I data exhibitlarger forbidden velocities over a wider longitude range than are seen inmolecular gas; this important difference is the reason our favored modeldiffers so significantly from other recently proposed models.[Journal_ref: Astrophys.J.524:112-128,1999]
• Weiner, B. J., & Williams, T. B. (1996). Detection of H-alpha emission from the Magellanic Stream: evidence for an extended gaseous Galactic halo. Astron.J., 111, 1156-1163.
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  We have detected faint, diffuse H$\alpha emission from several points alongthe Magellanic Stream, using the Rutgers Fabry--Perot Interferometer at theCTIO 1.5-m telescope. At points on the leading edges of the H I clouds MS II,MS III, and MS IV, we detect H$\alpha emission of surface brightness $0.37 \pm0.02$ Rayleighs, $0.21 \pm 0.04$ R, and $0.20 \pm 0.02$ R respectively,corresponding to emission measures of 1.0 to 0.5 \cmsixpc. We have observedseveral positions near the MS IV concentration, and find that the strongestemission is on the sharp leading-edge density gradient. There is less emissionat points away from the gradient, and halfway between MS III and MS IV theH$\alpha surface brightness is $< 0.04$ R. We attribute the H$\alpha emission at cloud leading edges to heating of theStream clouds by ram pressure from ionized gas in the halo of the Galaxy. Theseobservations suggest that ram pressure from halo gas plays a large role instripping the Stream out of the Magellanic Clouds. They also suggest thepresence of a relatively large density of gas, $n_{\rm H} \sim 10^{-4}cm^{-3}$, in the Galactic halo at $\sim 50$ kpc radius, and far above theGalactic plane, $b \sim -80\deg$. This implies that the Galaxy has a very largebaryonic, gaseous extent, and supports models of Lyman-$\alpha and metal-lineQSO absorption lines in which the absorption systems reside in extendedgalactic halos.[Journal_ref: Astron.J.111:1156-1163,1996]

Proceedings Publications

• Pearce, E. C., & Weiner, B. J. (2019, september). Examining the Effects of On-Orbit Aging of SL-12 Rocket Bodies using Visible Band Spectra with the MMT Telescope. In Advanced Maui Optical and Space Surveillance Technologies (AMOS) Conference.
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  The characterization of deep space debris has posed a significant challenge in SSA. To be most operationally effective, characterization must be performed quickly and under non-ideal operational conditions, generally using non-resolved techniques. The use of multi-color photometry and the resultant color indices offer the potential to rapidly discriminate between debris and intact space objects such as rocket bodies and satellites. However, these studies are not well informed by high resolution spectra of these same objects due to the lack of prior measurements with large astronomical telescopes. High resolution spectroscopy is not routinely collected by our SSA network. Nonetheless, several researchers have collected satellite spectra for research purposes. Several researchers have also noted the progressive reddening of spacecraft surfaces. Jorgensen measured reflectance spectra over a range of years on orbit (YOO) of 10-13 years of foreign discarded rocket bodies and noted significant increase in relative reflectance above 750 nm. Similarly, aging has been noted on GPS payloads using BVRI photometry by Fliegel.In this study, we have collected high resolution spectra of a group of five Russian SL-12 rocket bodies in geosynchronous orbit. The spectra were collected with the Blue Channel Spectrograph on the 6.5 m MMT telescope at Mt. Hopkins. The measurements were taken using the 300-line grating, which is blazed for the red, and can cover a 5200 Å range at dispersion 1.96 Å/pixel. The large collecting aperture of the MMT allowed the rapid collection of multiple high signal-to-noise spectra with only 2 minutes per exposure. This short exposure allowed us to have confidence the solar phase angle was near constant during each collection, but that the spectra were averaged over the rotation of the rocket body. These spectra allow analysis of both the variation in albedo over a large wavelength range, and searches for discrete absorption features. The SL-12 (also called the “Proton K”) was a mainstay Russian four-stage to GEO launch vehicle that was used from 1974 to 2012 (Gunter 2017). The SL-12 fourth stage rocket bodies (henceforth referred to as “SL-12 RB”) offer a convenient ensemble of objects for which photometric techniques can be developed and tested. For this study, five SL-12s with a range of years-on-orbit (YOO) ranging from 23-35 years were collected, allowing a comparative study of the evolution of the spectra over a 12-year difference in age. Additionally, all these objects have been previously observed with the UKIRT WFCAM. The spectra are analyzed for evidence of the effects of on-orbit reddening and other changes over time.
• Pearce, E., Weiner, B., Block, A., Krantz, H., Rockowitz, K., Sease, B., Hennessy, G., & Wilson, M. (2019, sep). Examining the Effects of On-Orbit Aging of SL-12 Rocket Bodies using Visible Band Spectra with the MMT Telescope and 5-Color Photometry with the UKIRT/WFCAM. In Proceedings of the Advanced Maui Optical and Space Surveillance Technologies Conference.
• Weiner, B. J., Sand, D., Gabor, P., Johnson, C., Swindell, S., Kub{\'anek}, P., Gasho, V., Golota, T., Jannuzi, B., Milne, P., Smith, N., & Zaritsky, D. (2018, Jul). Development of the Arizona Robotic Telescope Network. In Observatory Operations: Strategies, Processes, and Systems VII, 10704.
• Hart, M., Hart, M., Furfaro, R., Furfaro, R., Weiner, B. J., Weiner, B. J., Corral, E. L., Corral, E. L., Lyons, E. H., Lyons, E. H., Surdeanu, M., Surdeanu, M., Butcher, E., Butcher, E., Gaylor, D., Gaylor, D., Jah, M. K., Jah, M. K., Merchant, N. C., , Merchant, N. C., et al. (2016, May). A New Approach to Space Domain Awareness at the University of Arizona. In NATO Symposium on Considerations for Space and Space-Enabled Capabilities in NATO Coalition Operations, SCI-283.
• Hart, M., Hart, M., Hart, M., Hart, M., Jah, M. K., Jah, M. K., Jah, M. K., Jah, M. K., Gaylor, D., Gaylor, D., Gaylor, D., Gaylor, D., Butcher, E., Butcher, E., Butcher, E., Butcher, E., Ten Eyck, B., Ten Eyck, B., Ten Eyck, B., , Ten Eyck, B., et al. (2016, May). A New Approach to Space Domain Awareness at the University of Arizona. In NATO Symposium on "Considerations for Space and Space-Enabled Capabilities in NATO Coalition Operations".
• {Simons}, R., {Kassin}, S., {Trump}, J., {Weiner}, B., {Barro}, G., {Koo}, D., {Faber}, S., , Y. (2015, aug). "{When are Galaxy Disks Formed? Multi-PA Galaxy Kinematics at z~{}2 with Keck/MOSFIRE}". In IAU General Assembly, 22, 2257477.
• Alberts, S., Pope, A., Brodwin, M., Atlee, D. W., Lin, Y., Chary, R., Dey, A., Eisenhardt, P. R., Gettings, D., Gonzalez, A. H., Jannuzi, B., Mancone, C., Moustakas, J., Snyder, G. F., Stanford, S. A., Stern, D., Weiner, B. J., & Zeimann, G. (2014, jan). How Environment Affects Star Formation: Tracing Activity in High Redshift Galaxy Clusters. In American Astronomical Society Meeting Abstracts, 223, #130.02.
• Mei, S., Scarlata, C., Pentericci, L., Newman, J., Teplitz, H. I., Weiner, B. J., Ashby, M., Castellano, M., Conselice, C., Finkelstein, S. L., Galametz, A., Koekemoer, A. M., Lucas, R. A., Rafelski, M., & Team, C. (2014, jan). A progenitor of today rsquos typical galaxy clusters at z=1.84. In American Astronomical Society Meeting Abstracts, 223, #145.08.
• Simons, R., Kassin, S. A., Weiner, B. J., & Lee, J. C. (2014, jan). A Characteristic Mass in the Low Redshift Tully Fisher Relation. In American Astronomical Society Meeting Abstracts, 223, #205.04.
• Trump, J. R., Brandt, W. N., Weiner, B. J., Juneau, S., CANDELS, ., & 3D-HST, . (2014, jan). The AGN Census at Cosmic Noon: the Unbiased Galaxy-AGN Connection from Spatially Resolved Line Ratios. In American Astronomical Society Meeting Abstracts, 223, #402.05.
• Weiner, B. J. (2014, jan). Occupy Hard Drives: Making your work more valuable by giving it away. In American Astronomical Society Meeting Abstracts, 223, #225.01.
• Weiner, B. J., & Team, A. (2014, jan). Star formation rates and extinction at z=1-2 from the AGHAST HST infrared grism survey. In American Astronomical Society Meeting Abstracts, 223, #227.07.
• Kassin, S. A., Weiner, B. J., Faber, S. M., Gardner, J. P., & Team, D. (2013, jan). The Epoch of Disk Settling: 1 to Today. In American Astronomical Society Meeting Abstracts, 221, #304.06.
• Mostek, N. J., Coil, A. L., Cooper, M. C., Davis, M., Newman, J., & Weiner, B. J. (2013, jan). The DEEP2 Galaxy Redshift Survey: Clustering Dependence on Galaxy Stellar Mass and Star Formation Rate at 1. In American Astronomical Society Meeting Abstracts, 221, #434.01.
• Trump, J. R., Barro, G., Weiner, B. J., Konidaris, N., Koo, D. C., Kocevski, D., Yan, R., Juneau, S., Faber, S. M., & CANDELS, . (2013, jan). Do z gt1 Clumpy Galaxies in CANDELS Fuel AGNs?. In American Astronomical Society Meeting Abstracts, 221, #133.07.
• Hibon, P. M., Rhoads, J. E., Malhotra, S., Cooper, M., & Weiner, B. (2012, jan). A Lyman-Alpha Galaxy at Redshift z=6.944. In American Astronomical Society Meeting Abstracts #219, 219, #246.31.
• Ono, Y., Ouchi, M., Mobasher, B., Dickinson, M., Penner, K., Shimasaku, K., Weiner, B. J., Kartaltepe, J. S., Nakajima, K., Nayyeri, H., Stern, D., Kashikawa, N., & Spinrad, H. (2012, may). Spectroscopic Confirmation of Three z-Dropout Galaxies at z = 6.844-7.213: Demographics of Lya Emission in z sim 7 Galaxies. In American Astronomical Society Meeting Abstracts #220, 220, #429.03.
• Sheth, K., Melbourne, J., Kassin, S., Elmegreen, D. M., Elmegreen, B. G., Athanassoula, E., Abraham, R. G., Ellis, R. S., & Weiner, B. (2012, may). A Plausible Explanation for the Steep Redshift Decline in Barred Spirals: Dynamically Hot Disks. In American Astronomical Society Meeting Abstracts #220, 220, #409.05.
• Shipley, H. V., Papovich, C., Dey, A., Jannuzi, B., Rieke, G., & Weiner, B. (2012, jan). Spitzer Infrared Spectrograph Observations of Infrared-Luminous Galaxies at Moderate Redshift: Diagnostics of AGN and Star Formation. In American Astronomical Society Meeting Abstracts #219, 219, #246.17.
• Trump, J. R., Weiner, B. J., Koo, D. C., Faber, S. M., & Kocevski, D. D. (2012, jan). Emission-Line Diagnostics of Nuclear Activity and Star Formation in Galaxies at 0 ltz $ epsilon$ with CANDELS. In American Astronomical Society Meeting Abstracts #219, 219, #131.01.
• Weiner, B. J. (2012, jan). Infrared Spectroscopy with HST: Grism Results in the CANDELS Fields. In American Astronomical Society Meeting Abstracts #219, 219, #406.06.