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51. CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

Author

Grogin, Norman A., Kocevski, Dale D., Faber, S. M., Ferguson, Henry C., Koekemoer, Anton M., Riess, Adam G., Acquaviva, Viviana, Alexander, David M., Almaini, Omar, Ashby, Matthew L. N., Barden, Marco, Bell, Eric F., Bournaud, Frédéric, Brown, Thomas M., Caputi, Karina I., Casertano, Stefano, Cassata, Paolo, Castellano, Marco, Challis, Peter, Chary, Ranga-Ram, Cheung, Edmond, Cirasuolo, Michele, Conselice, Christopher J., Cooray, Asantha Roshan, Croton, Darren J., Daddi, Emanuele, Dahlen, Tomas, Davé, Romeel, de Mello, Duília F., Dekel, Avishai, Dickinson, Mark, Dolch, Timothy, Donley, Jennifer L., Dunlop, James S., Dutton, Aaron A., Elbaz, David, Fazio, Giovanni G., Filippenko, Alexei V., Finkelstein, Steven L., Fontana, Adriano, Gardner, Jonathan P., Garnavich, Peter M., Gawiser, Eric, Giavalisco, Mauro, Grazian, Andrea, Guo, Yicheng, Hathi, Nimish P., Häussler, Boris, Hopkins, Philip F., Huang, Jia-Sheng, Huang, Kuang-Han, Jha, Saurabh W., Kartaltepe, Jeyhan S., Kirshner, Robert P., Koo, David C., Lai, Kamson, Lee, Kyoung-Soo, Li, Weidong, Lotz, Jennifer M., Lucas, Ray A., Madau, Piero, McCarthy, Patrick J., McGrath, Elizabeth J., McIntosh, Daniel H., McLure, Ross J., Mobasher, Bahram, Moustakas, Leonidas A., Mozena, Mark, Nandra, Kirpal, Newman, Jeffrey A., Niemi, Sami-Matias, Noeske, Kai G., Papovich, Casey J., Pentericci, Laura, Pope, Alexandra, Primack, Joel R., Rajan, Abhijith, Ravindranath, Swara, Reddy, Naveen A., Renzini, Alvio, Rix, Hans-Walter, Robaina, Aday R., Rodney, Steven A., Rosario, David J., Rosati, Piero, Salimbeni, Sara, Scarlata, Claudia, Siana, Brian, Simard, Luc, Smidt, Joseph, Somerville, Rachel S., Spinrad, Hyron, Straughn, Amber N., Strolger, Louis-Gregory, Telford, Olivia, Teplitz, Harry I., Trump, Jonathan R., van der Wel, Arjen, Villforth, Carolin, Wechsler, Risa H., Weiner, Benjamin J., Wiklind, Tommy, Wild, Vivienne, Wilson, Grant, Wuyts, Stijn, Yan, Hao-Jing, and Yun, Min S.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) is designed to document the first third of galactic evolution, over the approximate redshift (z) range 8--1.5. It will image >250,000 distant galaxies using three separate cameras on the Hubble Space Telescope, from the mid-ultraviolet to the near-infrared, and will find and measure Type Ia supernovae at z>1.5 to test their accuracy as standardizable candles for cosmology. Five premier multi-wavelength sky regions are selected, each with extensive ancillary data. The use of five widely separated fields mitigates cosmic variance and yields statistically robust and complete samples of galaxies down to a stellar mass of 10^9 M_\odot to z \approx 2, reaching the knee of the ultraviolet luminosity function (UVLF) of galaxies to z \approx 8. The survey covers approximately 800 arcmin^2 and is divided into two parts. The CANDELS/Deep survey (5\sigma\ point-source limit H=27.7 mag) covers \sim 125 arcmin^2 within GOODS-N and GOODS-S. The CANDELS/Wide survey includes GOODS and three additional fields (EGS, COSMOS, and UDS) and covers the full area to a 5\sigma\ point-source limit of H \gtrsim 27.0 mag. Together with the Hubble Ultra Deep Fields, the strategy creates a three-tiered "wedding cake" approach that has proven efficient for extragalactic surveys. Data from the survey are nonproprietary and are useful for a wide variety of science investigations. In this paper, we describe the basic motivations for the survey, the CANDELS team science goals and the resulting observational requirements, the field selection and geometry, and the observing design. The Hubble data processing and products are described in a companion paper., Comment: Submitted to Astrophysical Journal Supplement Series; Revised version, subsequent to referee report

Published
2011
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52. The Majority of Compact Massive Galaxies at z~2 are Disk Dominated

Author

van der Wel, Arjen, Rix, Hans-Walter, Wuyts, Stijn, McGrath, Elizabeth J., Koekemoer, Anton M., Bell, Eric F., Holden, Bradford P., Robaina, Aday R., and McIntosh, Daniel H.

Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract

We investigate the stellar structure of massive, quiescent galaxies at z~2, based on Hubble Space Telescope/WFC3 imaging from the Early Release Science program. Our sample of 14 galaxies has stellar masses of M* > 10^{10.8} Msol and photometric redshifts of 1.5 < z < 2.5. In agreement with previous work, their half-light radii are <2 kpc, much smaller than equally massive galaxies in the present-day universe. A significant subset of the sample appears highly flattened in projection, which implies, considering viewing angle statistics, that a significant fraction of the galaxies in our sample have pronounced disks. This is corroborated by two-dimensional surface brightness profile fits. We estimate that 65% +/- 15% of the population of massive, quiescent z~2 galaxies are disk-dominated. The median disk scale length is 1.5 kpc, substantially smaller than the disks of equally massive galaxies in the present-day universe. Our results provide strong observational evidence that the much-discussed ultra-dense high-redshift galaxies should generally be thought of as disk-like stellar systems with the majority of stars formed from gas that had time to settle into a disk., Comment: published version

Published
2011
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53. Lens Inquiry: An Astronomy Lab for Non-science Majors at Hartnell Community College

Author

Putnam, Nicole M., Cheng, Judy Y., McGrath, Elizabeth J., Lai, David K., and Moth, Pimol

Subjects
Physics - Physics Education, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We describe a three hour inquiry activity involving converging lenses and telescopes as part of a semester-long astronomy lab course for non-science majors at Hartnell Community College in Salinas, CA. Students were shown several short demonstrations and given the chance to experiment with the materials, after which there was a class discussion about the phenomena they observed. Students worked in groups of 2-4 to design their own experiments to address a particular question of interest to them and then presented their findings to the class. An instructor-led presentation highlighted the students' discoveries and the lab's content goals, followed by a short worksheet-based activity that guided them in applying their new knowledge to build a simple telescope using two converging lenses. The activity was successful in emphasizing communication skills and giving students opportunities to engage in the process of science in different ways. One of the biggest challenges in designing this activity was covering all of the content given the short amount of time available. Future implementations may have more success by splitting the lab into two sessions, one focusing on converging lenses and the other focusing on telescopes., Comment: 11 pages, 3 figures, in ASP Conference Series 436, Learning from Inquiry in Practice, eds. L. Hunter and A. J. Metevier (San Francisco, CA: ASP), 333

Published
2010

54. Obscured Starburst Activity in High Redshift Clusters and Groups

Author

Kocevski, Dale D., Lemaux, Brian C., Lubin, Lori M., Gal, Roy R., McGrath, Elizabeth J., Fassnacht, Christopher D., Squires, Gordon K., Surace, Jason A., and Lacy, Mark

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Using Spitzer-MIPS 24um imaging and Keck spectroscopy we examine the nature of the obscured star forming population in three clusters and three groups at z~0.9. These six systems are components of the Cl1604 supercluster, the largest structure imaged by Spitzer at redshifts near unity. We find that the average density of 24um-detected galaxies within the Cl1604 clusters is nearly twice that of the surrounding field and that this overdensity scales with the cluster's dynamical state. The 24um-bright members often appear optically unremarkable and exhibit only moderate [OII] line emission due to severe obscuration. Their spatial distribution suggests they are an infalling population, but an examination of their spectral properties, morphologies and optical colors indicate they are not simply analogs of the field population that have yet to be quenched. Using stacked composite spectra, we find the 24um-detected cluster and group galaxies exhibit elevated levels of Balmer absorption compared to galaxies undergoing normal, continuous star formation. A similar excess is not observed in field galaxies with equivalent infrared luminosities, indicating a greater fraction of the detected cluster and group members have experienced a burst of star formation in the recent past compared to their counterparts in the field. Our results suggest that gas-rich galaxies at high redshift experience a temporary increase in their star formation activity as they assemble into denser environments. Using HST-ACS imaging we find that disturbed morphologies are common among the 24um-detected cluster and group members and become more prevalent in regions of higher galaxy density. We conclude that mergers are the dominant triggering mechanism responsible for the enhanced star formation found in the Cl1604 groups, while a mix of harassment and mergers are likely driving the activity of the cluster galaxies., Comment: 18 pages, 19 figures, submitted to ApJ

Published
2010
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55. Morphologies and Color Gradients of Luminous Evolved Galaxies at z~1.5

Author

McGrath, Elizabeth J., Stockton, Alan, Canalizo, Gabriela, Iye, Masanori, and Maihara, Toshinori

Subjects
Astrophysics
Abstract

We have examined in detail the morphologies of seven z~1.5 passively evolving luminous red galaxies using high resolution HST NICMOS and ACS imaging data. Almost all of these galaxies appear to be relaxed systems, with smooth morphologies at both rest-frame UV and visible wavelengths. Previous results from spectral synthesis modeling favor a single burst of star formation more than 1 Gyr before the observed epoch. The prevalence of old stellar populations, however, does not correlate exclusively with early-type morphologies as it does in the local universe; the light profiles for some of these galaxies appear to be dominated by massive exponential disks. This evidence for massive old disks, along with the apparent uniformity of stellar age across the disk, suggests formation by a mechanism better described as a form of monolithic collapse than as a hierarchical merger. These galaxies could not have undergone a single major merging event since the bulk of their stars were formed, more than 1 Gyr earlier. There is at least one case, however, that appears to be undergoing a "dry merger", which may be an example of the process that converts these unusual galaxies into the familiar spheroids that dominate galaxies comprising old stellar populations at the present epoch., Comment: 16 pages, 9 figures (8 in color), accepted for publication in ApJ

Published
2007
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56. Stellar Populations of Luminous Evolved Galaxies at z~1.5

Author

McGrath, Elizabeth J., Stockton, Alan, and Canalizo, Gabriela

Subjects
Astrophysics
Abstract

Observational evidence has been mounting over the past decade that at least some luminous (~2 L*) galaxies have formed nearly all of their stars within a short period of time only 1-2x10^9 years after the Big Bang. These are examples of the first major episodes of star formation in the Universe and provide insights into the formation of the earliest massive galaxies. We have examined in detail the stellar populations of six z~1.5 galaxies that appear to be passively evolving, using both ground and space-based photometry covering rest-frame UV to visible wavelengths. In addition, we have obtained medium-resolution spectroscopy for five of the six galaxies, covering the rest-frame UV portion of the spectrum. Spectral synthesis modeling for four of these galaxies favors a single burst of star formation more than 1 Gyr before the observed epoch. The other two exhibit slightly younger ages with a higher dust content and evidence for a small contribution from either recent star formation or active nuclei. The implied formation redshifts for the oldest of these sources are consistent with previous studies of passive galaxies at high redshift, and improved stellar modeling has shown these results to be quite robust. It now seems clear that any valid galaxy formation scenario must be able to account for these massive (2x10^11 M_sun) galaxies at very early times in the Universe., Comment: 10 pages, 3 figures (2 in color), accepted for publication in ApJ

Published
2007
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57. A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars

Author

Larson, Rebecca L., primary, Finkelstein, Steven L., additional, Kocevski, Dale D., additional, Hutchison, Taylor A., additional, Trump, Jonathan R., additional, Haro, Pablo Arrabal, additional, Bromm, Volker, additional, Cleri, Nikko J., additional, Dickinson, Mark, additional, Fujimoto, Seiji, additional, Kartaltepe, Jeyhan S., additional, Koekemoer, Anton M., additional, Papovich, Casey, additional, Pirzkal, Nor, additional, Tacchella, Sandro, additional, Zavala, Jorge A., additional, Bagley, Micaela, additional, Behroozi, Peter, additional, Champagne, Jaclyn B., additional, Cole, Justin W., additional, Jung, Intae, additional, Morales, Alexa M., additional, Yang, Guang, additional, Zhang, Haowen, additional, Zitrin, Adi, additional, Amorín, Ricardo O., additional, Burgarella, Denis, additional, Casey, Caitlin M., additional, Chávez Ortiz, Óscar A., additional, Cox, Isabella G., additional, Chworowsky, Katherine, additional, Fontana, Adriano, additional, Gawiser, Eric, additional, Grazian, Andrea, additional, Grogin, Norman A., additional, Harish, Santosh, additional, Hathi, Nimish P., additional, Hirschmann, Michaela, additional, Holwerda, Benne W., additional, Juneau, Stéphanie, additional, Leung, Gene C. K., additional, Lucas, Ray A., additional, McGrath, Elizabeth J., additional, Pérez-González, Pablo G., additional, Rigby, Jane R., additional, Seillé, Lise-Marie, additional, Simons, Raymond C., additional, de la Vega, Alexander, additional, Weiner, Benjamin J., additional, Wilkins, Stephen M., additional, and Yung, L. Y. Aaron, additional

Published
2023
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58. Hidden Little Monsters:Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS

Author

Kocevski, Dale D., Onoue, Masafusa, Inayoshi, Kohei, Trump, Jonathan R., Haro, Pablo Arrabal, Grazian, Andrea, Dickinson, Mark, Finkelstein, Steven L., Kartaltepe, Jeyhan S., Hirschmann, Michaela, Aird, James, Holwerda, Benne W., Fujimoto, Seiji, Juneau, Stéphanie, Amorín, Ricardo O., Backhaus, Bren E., Bagley, Micaela B., Barro, Guillermo, Bell, Eric F., Bisigello, Laura, Calabrò, Antonello, Cleri, Nikko J., Cooper, M. C., Ding, Xuheng, Grogin, Norman A., Ho, Luis C., Hutchison, Taylor A., Inoue, Akio K., Jiang, Linhua, Jones, Brenda, Koekemoer, Anton M., Li, Wenxiu, Li, Zhengrong, Mcgrath, Elizabeth J., Molina, Juan, Papovich, Casey, Pérez-gonzález, Pablo G., Pirzkal, Nor, Wilkins, Stephen M., Yang, Guang, Yung, L. Y. Aaron, Kocevski, Dale D., Onoue, Masafusa, Inayoshi, Kohei, Trump, Jonathan R., Haro, Pablo Arrabal, Grazian, Andrea, Dickinson, Mark, Finkelstein, Steven L., Kartaltepe, Jeyhan S., Hirschmann, Michaela, Aird, James, Holwerda, Benne W., Fujimoto, Seiji, Juneau, Stéphanie, Amorín, Ricardo O., Backhaus, Bren E., Bagley, Micaela B., Barro, Guillermo, Bell, Eric F., Bisigello, Laura, Calabrò, Antonello, Cleri, Nikko J., Cooper, M. C., Ding, Xuheng, Grogin, Norman A., Ho, Luis C., Hutchison, Taylor A., Inoue, Akio K., Jiang, Linhua, Jones, Brenda, Koekemoer, Anton M., Li, Wenxiu, Li, Zhengrong, Mcgrath, Elizabeth J., Molina, Juan, Papovich, Casey, Pérez-gonzález, Pablo G., Pirzkal, Nor, Wilkins, Stephen M., Yang, Guang, and Yung, L. Y. Aaron

Published
2023

59. CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST

Author

Kocevski, Dale D., Barro, Guillermo, McGrath, Elizabeth J., Finkelstein, Steven L., Bagley, Micaela B., Ferguson, Henry C., Jogee, Shardha, Yang, Guang, Dickinson, Mark, Hathi, Nimish P., Backhaus, Bren E., Bell, Eric F., Bisigello, Laura, Buat, Véronique, Burgarella, Denis, Casey, Caitlin M., Cleri, Nikko J., Cooper, M. C., Costantin, Luca, Croton, Darren, Daddi, Emanuele, Fontana, Adriano, Fujimoto, Seiji, Gardner, Jonathan P., Gawiser, Eric, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Guo, Yuchen, Haro, Pablo Arrabal, Hirschmann, Michaela, Holwerda, Benne W., Huertas-Company, Marc, Hutchison, Taylor A., Iyer, Kartheik G., Jones, Brenda, Juneau, Stéphanie, Kartaltepe, Jeyhan S., Kewley, Lisa J., Kirkpatrick, Allison, Koekemoer, Anton M., Kurczynski, Peter, Bail, Aurélien Le, Long, Arianna S., Lotz, Jennifer M., Lucas, Ray A., Papovich, Casey, Pentericci, Laura, Pérez-González, Pablo G., Pirzkal, Nor, Rafelski, Marc, Ravindranath, Swara, Somerville, Rachel S., Straughn, Amber N., Tacchella, Sandro, Trump, Jonathan R., Wilkins, Stephen M., Wuyts, Stijn, Aaron Yung, L. Y., Zavala, Jorge A., Kocevski, Dale D., Barro, Guillermo, McGrath, Elizabeth J., Finkelstein, Steven L., Bagley, Micaela B., Ferguson, Henry C., Jogee, Shardha, Yang, Guang, Dickinson, Mark, Hathi, Nimish P., Backhaus, Bren E., Bell, Eric F., Bisigello, Laura, Buat, Véronique, Burgarella, Denis, Casey, Caitlin M., Cleri, Nikko J., Cooper, M. C., Costantin, Luca, Croton, Darren, Daddi, Emanuele, Fontana, Adriano, Fujimoto, Seiji, Gardner, Jonathan P., Gawiser, Eric, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Guo, Yuchen, Haro, Pablo Arrabal, Hirschmann, Michaela, Holwerda, Benne W., Huertas-Company, Marc, Hutchison, Taylor A., Iyer, Kartheik G., Jones, Brenda, Juneau, Stéphanie, Kartaltepe, Jeyhan S., Kewley, Lisa J., Kirkpatrick, Allison, Koekemoer, Anton M., Kurczynski, Peter, Bail, Aurélien Le, Long, Arianna S., Lotz, Jennifer M., Lucas, Ray A., Papovich, Casey, Pentericci, Laura, Pérez-González, Pablo G., Pirzkal, Nor, Rafelski, Marc, Ravindranath, Swara, Somerville, Rachel S., Straughn, Amber N., Tacchella, Sandro, Trump, Jonathan R., Wilkins, Stephen M., Wuyts, Stijn, Aaron Yung, L. Y., and Zavala, Jorge A.

Abstract

We report on the host properties of five X-ray-luminous active galactic nuclei (AGN) identified at 3 < z < 5 in the first epoch of imaging from the Cosmic Evolution Early Release Science Survey. Each galaxy has been imaged with the JWST Near-Infrared Camera, which provides rest-frame optical morphologies at these redshifts. We also derive stellar masses and star formation rates for each host by fitting its spectral energy distribution using a combination of galaxy and AGN templates. We find that three of the AGN hosts have spheroidal morphologies, one is a bulge-dominated disk, and one is dominated by pointlike emission. None are found to show strong morphological disturbances that might indicate a recent interaction or merger event. When compared to a sample of mass-matched inactive galaxies, we find that the AGN hosts have morphologies that are less disturbed and more bulge-dominated. Notably, all four of the resolved hosts have rest-frame optical colors consistent with a quenched or poststarburst stellar population. The presence of AGN in passively evolving galaxies at z > 3 is significant because a rapid feedback mechanism is required in most semianalytic models and cosmological simulations to explain the growing population of massive quiescent galaxies observed at these redshifts. Our findings show that AGN can continue to inject energy into these systems after their star formation is curtailed, potentially heating their halos and preventing renewed star formation. Additional observations will be needed to determine what role this feedback may play in helping to quench these systems and/or maintain their quiescent state.

Published
2023

60. Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at $z=4$ to $8$ from CEERS

Author

Chworowsky, Katherine, Finkelstein, Steven L., Boylan-Kolchin, Michael, McGrath, Elizabeth J., Iyer, Kartheik G., Papovich, Casey, Dickinson, Mark, Taylor, Anthony J., Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Micaela B., Backhaus, Bren E., Bhatawdekar, Rachana, Cheng, Yingjie, Cleri, Nikko J., Cole, Justin W., Cooper, M. C., Costantin, Luca, Dekel, Avishai, Franco, Maximilien, Fujimoto, Seiji, Hayward, Christopher C., Holwerda, Benne W., Huertas-Company, Marc, Hirschmann, Michaela, Hutchison, Taylor A., Koekemoer, Anton M., Larson, Rebecca L., Li, Zhaozhou, Long, Arianna S., Lucas, Ray A., Pirzkal, Nor, Rodighiero, Giulia, Somerville, Rachel S., Vanderhoof, Brittany N., de la Vega, Alexander, Wilkins, Stephen M., Yang, Guang, Zavala, Jorge A., Chworowsky, Katherine, Finkelstein, Steven L., Boylan-Kolchin, Michael, McGrath, Elizabeth J., Iyer, Kartheik G., Papovich, Casey, Dickinson, Mark, Taylor, Anthony J., Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Micaela B., Backhaus, Bren E., Bhatawdekar, Rachana, Cheng, Yingjie, Cleri, Nikko J., Cole, Justin W., Cooper, M. C., Costantin, Luca, Dekel, Avishai, Franco, Maximilien, Fujimoto, Seiji, Hayward, Christopher C., Holwerda, Benne W., Huertas-Company, Marc, Hirschmann, Michaela, Hutchison, Taylor A., Koekemoer, Anton M., Larson, Rebecca L., Li, Zhaozhou, Long, Arianna S., Lucas, Ray A., Pirzkal, Nor, Rodighiero, Giulia, Somerville, Rachel S., Vanderhoof, Brittany N., de la Vega, Alexander, Wilkins, Stephen M., Yang, Guang, and Zavala, Jorge A.

Abstract

We analyze the evolution of massive (log$_{10}$ [$M_\star/M_\odot$] $>10$) galaxies at $z \sim$ 4--8 selected from the JWST Cosmic Evolution Early Release Science (CEERS) survey. We infer the physical properties of all galaxies in the CEERS NIRCam imaging through spectral energy distribution (SED) fitting with dense basis to select a sample of high redshift massive galaxies. Where available we include constraints from additional CEERS observing modes, including 18 sources with MIRI photometric coverage, and 28 sources with spectroscopic confirmations from NIRSpec or NIRCam wide-field slitless spectroscopy. We sample the recovered posteriors in stellar mass from SED fitting to infer the volume densities of massive galaxies across cosmic time, taking into consideration the potential for sample contamination by active galactic nuclei (AGN). We find that the evolving abundance of massive galaxies tracks expectations based on a constant baryon conversion efficiency in dark matter halos for $z \sim$ 1--4. At higher redshifts, we observe an excess abundance of massive galaxies relative to this simple model. These higher abundances can be explained by modest changes to star formation physics and/or the efficiencies with which star formation occurs in massive dark matter halos, and are not in tension with modern cosmology., Comment: 20 pages, 10 figures

Published
2023

61. A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang:Identifying a Progenitor of Massive z > 6 Quasars

Author

Larson, Rebecca L., Finkelstein, Steven L., Kocevski, Dale D., Hutchison, Taylor A., Trump, Jonathan R., Arrabal Haro, Pablo, Bromm, Volker, Cleri, Nikko J., Dickinson, Mark, Fujimoto, Seiji, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Papovich, Casey, Pirzkal, Nor, Tacchella, Sandro, Zavala, Jorge A., Bagley, Micaela, Behroozi, Peter, Champagne, Jaclyn B., Cole, Justin W., Jung, Intae, Morales, Alexa M., Yang, Guang, Zhang, Haowen, Zitrin, Adi, Amorín, Ricardo O., Burgarella, Denis, Casey, Caitlin M., Chávez Ortiz, Óscar A., Cox, Isabella G., Chworowsky, Katherine, Fontana, Adriano, Gawiser, Eric, Grazian, Andrea, Grogin, Norman A., Harish, Santosh, Hathi, Nimish P., Hirschmann, Michaela, Holwerda, Benne W., Juneau, Stéphanie, Leung, Gene C. K., Lucas, Ray A., Mcgrath, Elizabeth J., Pérez-gonzález, Pablo G., Rigby, Jane R., Seillé, Lise-marie, Simons, Raymond C., De La Vega, Alexander, Weiner, Benjamin J., Wilkins, Stephen M., Yung, L. Y. Aaron, Larson, Rebecca L., Finkelstein, Steven L., Kocevski, Dale D., Hutchison, Taylor A., Trump, Jonathan R., Arrabal Haro, Pablo, Bromm, Volker, Cleri, Nikko J., Dickinson, Mark, Fujimoto, Seiji, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Papovich, Casey, Pirzkal, Nor, Tacchella, Sandro, Zavala, Jorge A., Bagley, Micaela, Behroozi, Peter, Champagne, Jaclyn B., Cole, Justin W., Jung, Intae, Morales, Alexa M., Yang, Guang, Zhang, Haowen, Zitrin, Adi, Amorín, Ricardo O., Burgarella, Denis, Casey, Caitlin M., Chávez Ortiz, Óscar A., Cox, Isabella G., Chworowsky, Katherine, Fontana, Adriano, Gawiser, Eric, Grazian, Andrea, Grogin, Norman A., Harish, Santosh, Hathi, Nimish P., Hirschmann, Michaela, Holwerda, Benne W., Juneau, Stéphanie, Leung, Gene C. K., Lucas, Ray A., Mcgrath, Elizabeth J., Pérez-gonzález, Pablo G., Rigby, Jane R., Seillé, Lise-marie, Simons, Raymond C., De La Vega, Alexander, Weiner, Benjamin J., Wilkins, Stephen M., and Yung, L. Y. Aaron

Published
2023

62. A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging

Author

Finkelstein, Steven L., Bagley, Micaela B., Haro, Pablo Arrabal, Dickinson, Mark, Ferguson, Henry C., Kartaltepe, Jeyhan S., Papovich, Casey, Burgarella, Denis, Kocevski, Dale D., Huertas-Company, Marc, Iyer, Kartheik G., Koekemoer, Anton M., Larson, Rebecca L., Pérez-González, Pablo G., Rose, Caitlin, Tacchella, Sandro, Wilkins, Stephen M., Chworowsky, Katherine, Medrano, Aubrey, Morales, Alexa M., Somerville, Rachel S., Yung, L. Y. Aaron, Fontana, Adriano, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Kewley, Lisa J., Kirkpatrick, Allison, Kurczynski, Peter, Lotz, Jennifer M., Pentericci, Laura, Pirzkal, Nor, Ravindranath, Swara, Ryan, Russell E., Jr., Trump, Jonathan R., Yang, Guang, and The CEERS Team, Almaini, Omar, Amorín, Ricardo O., Annunziatella, Marianna, Backhaus, Bren E., Barro, Guillermo, Behroozi, Peter, Bell, Eric F., Bhatawdekar, Rachana, Bisigello, Laura, Bromm, Volker, Buat, Véronique, Buitrago, Fernando, Calabrò, Antonello, Casey, Caitlin M., Castellano, Marco, Chávez Ortiz, Óscar A., Ciesla, Laure, Cleri, Nikko J., Cohen, Seth H., Cole, Justin W., Cooke, Kevin C., Cooper, M. C., Cooray, Asantha R., Costantin, Luca, Cox, Isabella G., Croton, Darren, Daddi, Emanuele, Davé, Romeel, de la Vega, Alexander, Dekel, Avishai, Elbaz, David, Estrada-Carpenter, Vicente, Faber, Sandra M., Fernández, Vital, Finkelstein, Keely D., Freundlich, Jonathan, Fujimoto, Seiji, García-Argumánez, Ángela, Gardner, Jonathan P., Gawiser, Eric, Gómez-Guijarro, Carlos, Guo, Yuchen, Hamblin, Kurt, Hamilton, Timothy S., Hathi, Nimish P., Holwerda, Benne W., Hirschmann, Michaela, Hutchison, Taylor A., Jaskot, Anne E., Jha, Saurabh W., Jogee, Shardha, Juneau, Stéphanie, Jung, Intae, Kassin, Susan A., Bail, Aurélien Le, Leung, Gene C. K., Lucas, Ray A., Magnelli, Benjamin, Mantha, Kameswara Bharadwaj, Matharu, Jasleen, McGrath, Elizabeth J., McIntosh, Daniel H., Merlin, Emiliano, Mobasher, Bahram, Newman, Jeffrey A., Nicholls, David C., Pandya, Viraj, Rafelski, Marc, Ronayne, Kaila, Santini, Paola, Seillé, Lise-Marie, Shah, Ekta A., Shen, Lu, Simons, Raymond C., Snyder, Gregory F., Stanway, Elizabeth R., Straughn, Amber N., Teplitz, Harry I., Vanderhoof, Brittany N., Vega-Ferrero, Jesús, Wang, Weichen, Weiner, Benjamin J., Willmer, Christopher N. A., Wuyts, Stijn, Zavala, Jorge A., Finkelstein, Steven L. [0000-0001-8519-1130], Bagley, Micaela B. [0000-0002-9921-9218], Haro, Pablo Arrabal [0000-0002-7959-8783], Dickinson, Mark [0000-0001-5414-5131], Ferguson, Henry C. [0000-0001-7113-2738], Kartaltepe, Jeyhan S. [0000-0001-9187-3605], Papovich, Casey [0000-0001-7503-8482], Burgarella, Denis [0000-0002-4193-2539], Kocevski, Dale D. [0000-0002-8360-3880], Huertas-Company, Marc [0000-0002-1416-8483], Iyer, Kartheik G. [0000-0001-9298-3523], Koekemoer, Anton M. [0000-0002-6610-2048], Larson, Rebecca L. [0000-0003-2366-8858], Pérez-González, Pablo G. [0000-0003-4528-5639], Rose, Caitlin [0000-0002-8018-3219], Tacchella, Sandro [0000-0002-8224-4505], Wilkins, Stephen M. [0000-0003-3903-6935], Chworowsky, Katherine [0000-0003-4922-0613], Morales, Alexa M. [0000-0003-4965-0402], Somerville, Rachel S. [0000-0002-6748-6821], Yung, L. Y. Aaron [0000-0003-3466-035X], Fontana, Adriano [0000-0003-3820-2823], Giavalisco, Mauro [0000-0002-7831-8751], Grazian, Andrea [0000-0002-5688-0663], Grogin, Norman A. [0000-0001-9440-8872], Kewley, Lisa J. [0000-0001-8152-3943], Kirkpatrick, Allison [0000-0002-1306-1545], Kurczynski, Peter [0000-0002-8816-5146], Lotz, Jennifer M. [0000-0003-3130-5643], Pentericci, Laura [0000-0001-8940-6768], Pirzkal, Nor [0000-0003-3382-5941], Ravindranath, Swara [0000-0002-5269-6527], Ryan, Russell E., Jr. [0000-0003-0894-1588], Trump, Jonathan R. [0000-0002-1410-0470], Yang, Guang [0000-0001-8835-7722], Almaini, Omar [0000-0001-9328-3991], Amorín, Ricardo O. [0000-0001-5758-1000], Annunziatella, Marianna [0000-0002-8053-8040], Backhaus, Bren E. [0000-0001-8534-7502], Behroozi, Peter [0000-0002-2517-6446], Bell, Eric F. [0000-0002-5564-9873], Bhatawdekar, Rachana [0000-0003-0883-2226], Bisigello, Laura [0000-0003-0492-4924], Bromm, Volker [0000-0003-0212-2979], Buat, Véronique [0000-0003-3441-903X], Buitrago, Fernando [0000-0002-2861-9812], Calabrò, Antonello [0000-0003-2536-1614], Casey, Caitlin M. [0000-0002-0930-6466], Castellano, Marco [0000-0001-9875-8263], Chávez Ortiz, Óscar A. [0000-0003-2332-5505], Ciesla, Laure [0000-0003-0541-2891], Cleri, Nikko J. [0000-0001-7151-009X], Cohen, Seth H. [0000-0003-3329-1337], Cole, Justin W. [0000-0002-6348-1900], Cooke, Kevin C. [0000-0002-2200-9845], Cooper, M. C. [0000-0003-1371-6019], Cooray, Asantha R. [0000-0002-3892-0190], Costantin, Luca [0000-0001-6820-0015], Cox, Isabella G. [0000-0002-1803-794X], Croton, Darren [0000-0002-5009-512X], Daddi, Emanuele [0000-0002-3331-9590], Davé, Romeel [0000-0003-2842-9434], de la Vega, Alexander [0000-0002-6219-5558], Dekel, Avishai [0000-0003-4174-0374], Elbaz, David [0000-0002-7631-647X], Estrada-Carpenter, Vicente [0000-0001-8489-2349], Fernández, Vital [0000-0003-0531-5450], Finkelstein, Keely D. [0000-0003-0792-5877], Freundlich, Jonathan [0000-0002-5245-7796], Fujimoto, Seiji [0000-0001-7201-5066], García-Argumánez, Ángela [0000-0002-8365-5525], Gardner, Jonathan P. [0000-0003-2098-9568], Gawiser, Eric [0000-0003-1530-8713], Gómez-Guijarro, Carlos [0000-0002-4085-9165], Guo, Yuchen [0000-0002-4162-6523], Hamblin, Kurt [0000-0002-6292-4589], Hamilton, Timothy S. [0000-0002-9753-1769], Hathi, Nimish P. [0000-0001-6145-5090], Holwerda, Benne W. [0000-0002-4884-6756], Hirschmann, Michaela [0000-0002-3301-3321], Hutchison, Taylor A. [0000-0001-6251-4988], Jaskot, Anne E. [0000-0002-6790-5125], Jha, Saurabh W. [0000-0001-8738-6011], Jogee, Shardha [0000-0002-1590-0568], Juneau, Stéphanie [0000-0002-0000-2394], Jung, Intae [0000-0003-1187-4240], Kassin, Susan A. [0000-0002-3838-8093], Bail, Aurélien Le [0000-0002-9466-2763], Leung, Gene C. K. [0000-0002-9393-6507], Lucas, Ray A. [0000-0003-1581-7825], Magnelli, Benjamin [0000-0002-6777-6490], Matharu, Jasleen [0000-0002-7547-3385], McGrath, Elizabeth J. [0000-0001-8688-2443], Merlin, Emiliano [0000-0001-6870-8900], Newman, Jeffrey A. [0000-0001-8684-2222], Nicholls, David C. [0000-0003-0892-5203], Pandya, Viraj [0000-0002-2499-9205], Rafelski, Marc [0000-0002-9946-4731], Ronayne, Kaila [0000-0001-5749-5452], Santini, Paola [0000-0002-9334-8705], Seillé, Lise-Marie [0000-0001-7755-4755], Shah, Ekta A. [0000-0001-7811-9042], Shen, Lu [0000-0001-9495-7759], Simons, Raymond C. [0000-0002-6386-7299], Snyder, Gregory F. [0000-0002-4226-304X], Stanway, Elizabeth R. [0000-0002-8770-809X], Straughn, Amber N. [0000-0002-4772-7878], Teplitz, Harry I. [0000-0002-7064-5424], Vanderhoof, Brittany N. [0000-0002-8163-0172], Vega-Ferrero, Jesús [0000-0003-2338-5567], Wang, Weichen [0000-0002-9593-8274], Weiner, Benjamin J. [0000-0001-6065-7483], Willmer, Christopher N. A. [0000-0001-9262-9997], Wuyts, Stijn [0000-0003-3735-1931], and Apollo - University of Cambridge Repository

Subjects
Galaxies and Cosmology
Abstract

We report the discovery of a candidate galaxy with a photo-z of z ∼ 12 in the first epoch of the James Webb Space Telescope (JWST) Cosmic Evolution Early Release Science Survey. Following conservative selection criteria, we identify a source with a robust z phot = 11.8−0.2+0.3 (1σ uncertainty) with m F200W = 27.3 and ≳7σ detections in five filters. The source is not detected at λ < 1.4 μm in deep imaging from both Hubble Space Telescope (HST) and JWST and has faint ∼3σ detections in JWST F150W and HST F160W, which signal a Lyα break near the red edge of both filters, implying z ∼ 12. This object (Maisie’s Galaxy) exhibits F115W − F200W > 1.9 mag (2σ lower limit) with a blue continuum slope, resulting in 99.6% of the photo-z probability distribution function favoring z > 11. All data-quality images show no artifacts at the candidate’s position, and independent analyses consistently find a strong preference for z > 11. Its colors are inconsistent with Galactic stars, and it is resolved (r h = 340 ± 14 pc). Maisie’s Galaxy has log M */M ⊙ ∼ 8.5 and is highly star-forming (log sSFR ∼ −8.2 yr−1), with a blue rest-UV color (β ∼ −2.5) indicating little dust, though not extremely low metallicity. While the presence of this source is in tension with most predictions, it agrees with empirical extrapolations assuming UV luminosity functions that smoothly decline with increasing redshift. Should follow-up spectroscopy validate this redshift, our universe was already aglow with galaxies less than 400 Myr after the Big Bang.

Published
2022

63. First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging

Author

Guo, Yuchen, primary, Jogee, Shardha, additional, Finkelstein, Steven L., additional, Chen, Zilei, additional, Wise, Eden, additional, Bagley, Micaela B., additional, Barro, Guillermo, additional, Wuyts, Stijn, additional, Kocevski, Dale D., additional, Kartaltepe, Jeyhan S., additional, McGrath, Elizabeth J., additional, Ferguson, Henry C., additional, Mobasher, Bahram, additional, Giavalisco, Mauro, additional, Lucas, Ray A., additional, Zavala, Jorge A., additional, Lotz, Jennifer M., additional, Grogin, Norman A., additional, Huertas-Company, Marc, additional, Vega-Ferrero, Jesús, additional, Hathi, Nimish P., additional, Haro, Pablo Arrabal, additional, Dickinson, Mark, additional, Koekemoer, Anton M., additional, Papovich, Casey, additional, Pirzkal, Nor, additional, Yung, L. Y. Aaron, additional, Backhaus, Bren E., additional, Bell, Eric F., additional, Calabrò, Antonello, additional, Cleri, Nikko J., additional, Coogan, Rosemary T., additional, Cooper, M. C., additional, Costantin, Luca, additional, Croton, Darren, additional, Davis, Kelcey, additional, Dekel, Avishai, additional, Franco, Maximilien, additional, Gardner, Jonathan P., additional, Holwerda, Benne W., additional, Hutchison, Taylor A., additional, Pandya, Viraj, additional, Pérez-González, Pablo G., additional, Ravindranath, Swara, additional, Rose, Caitlin, additional, Trump, Jonathan R., additional, de la Vega, Alexander, additional, and Wang, Weichen, additional

Published
2023
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64. CEERS Key Paper. IV. A Triality in the Nature of HST-dark Galaxies

Author

Pérez-González, Pablo G., primary, Barro, Guillermo, additional, Annunziatella, Marianna, additional, Costantin, Luca, additional, García-Argumánez, Ángela, additional, McGrath, Elizabeth J., additional, Mérida, Rosa M., additional, Zavala, Jorge A., additional, Arrabal Haro, Pablo, additional, Bagley, Micaela B., additional, Backhaus, Bren E., additional, Behroozi, Peter, additional, Bell, Eric F., additional, Bisigello, Laura, additional, Buat, Véronique, additional, Calabrò, Antonello, additional, Casey, Caitlin M., additional, Cleri, Nikko J., additional, Coogan, Rosemary T., additional, Cooper, M. C., additional, Cooray, Asantha R., additional, Dekel, Avishai, additional, Dickinson, Mark, additional, Elbaz, David, additional, Ferguson, Henry C., additional, Finkelstein, Steven L., additional, Fontana, Adriano, additional, Franco, Maximilien, additional, Gardner, Jonathan P., additional, Giavalisco, Mauro, additional, Gómez-Guijarro, Carlos, additional, Grazian, Andrea, additional, Grogin, Norman A., additional, Guo, Yuchen, additional, Huertas-Company, Marc, additional, Jogee, Shardha, additional, Kartaltepe, Jeyhan S., additional, Kewley, Lisa J., additional, Kirkpatrick, Allison, additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Long, Arianna S., additional, Lotz, Jennifer M., additional, Lucas, Ray A., additional, Papovich, Casey, additional, Pirzkal, Nor, additional, Ravindranath, Swara, additional, Somerville, Rachel S., additional, Tacchella, Sandro, additional, Trump, Jonathan R., additional, Wang, Weichen, additional, Wilkins, Stephen M., additional, Wuyts, Stijn, additional, Yang, Guang, additional, and Yung, L. Y. Aaron, additional

Published
2023
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65. CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3–9 with JWST

Author

Kartaltepe, Jeyhan S., primary, Rose, Caitlin, additional, Vanderhoof, Brittany N., additional, McGrath, Elizabeth J., additional, Costantin, Luca, additional, Cox, Isabella G., additional, Yung, L. Y. Aaron, additional, Kocevski, Dale D., additional, Wuyts, Stijn, additional, Ferguson, Henry C., additional, Bagley, Micaela B., additional, Finkelstein, Steven L., additional, Amorín, Ricardo O., additional, Andrews, Brett H., additional, Arrabal Haro, Pablo, additional, Backhaus, Bren E., additional, Behroozi, Peter, additional, Bisigello, Laura, additional, Calabrò, Antonello, additional, Casey, Caitlin M., additional, Coogan, Rosemary T., additional, Cooper, M. C., additional, Croton, Darren, additional, de la Vega, Alexander, additional, Dickinson, Mark, additional, Fontana, Adriano, additional, Franco, Maximilien, additional, Grazian, Andrea, additional, Grogin, Norman A., additional, Hathi, Nimish P., additional, Holwerda, Benne W., additional, Huertas-Company, Marc, additional, Iyer, Kartheik G., additional, Jogee, Shardha, additional, Jung, Intae, additional, Kewley, Lisa J., additional, Kirkpatrick, Allison, additional, Koekemoer, Anton M., additional, Liu, James, additional, Lotz, Jennifer M., additional, Lucas, Ray A., additional, Newman, Jeffrey A., additional, Pacifici, Camilla, additional, Pandya, Viraj, additional, Papovich, Casey, additional, Pentericci, Laura, additional, Pérez-González, Pablo G., additional, Petersen, Jayse, additional, Pirzkal, Nor, additional, Rafelski, Marc, additional, Ravindranath, Swara, additional, Simons, Raymond C., additional, Snyder, Gregory F., additional, Somerville, Rachel S., additional, Stanway, Elizabeth R., additional, Straughn, Amber N., additional, Tacchella, Sandro, additional, Trump, Jonathan R., additional, Vega-Ferrero, Jesús, additional, Wilkins, Stephen M., additional, Yang, Guang, additional, and Zavala, Jorge A., additional

Published
2023
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66. CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST

Author

Kocevski, Dale D., primary, Barro, Guillermo, additional, McGrath, Elizabeth J., additional, Finkelstein, Steven L., additional, Bagley, Micaela B., additional, Ferguson, Henry C., additional, Jogee, Shardha, additional, Yang, Guang, additional, Dickinson, Mark, additional, Hathi, Nimish P., additional, Backhaus, Bren E., additional, Bell, Eric F., additional, Bisigello, Laura, additional, Buat, Véronique, additional, Burgarella, Denis, additional, Casey, Caitlin M., additional, Cleri, Nikko J., additional, Cooper, M. C., additional, Costantin, Luca, additional, Croton, Darren, additional, Daddi, Emanuele, additional, Fontana, Adriano, additional, Fujimoto, Seiji, additional, Gardner, Jonathan P., additional, Gawiser, Eric, additional, Giavalisco, Mauro, additional, Grazian, Andrea, additional, Grogin, Norman A., additional, Guo, Yuchen, additional, Arrabal Haro, Pablo, additional, Hirschmann, Michaela, additional, Holwerda, Benne W., additional, Huertas-Company, Marc, additional, Hutchison, Taylor A., additional, Iyer, Kartheik G., additional, Jones, Brenda, additional, Juneau, Stéphanie, additional, Kartaltepe, Jeyhan S., additional, Kewley, Lisa J., additional, Kirkpatrick, Allison, additional, Koekemoer, Anton M., additional, Kurczynski, Peter, additional, Bail, Aurélien Le, additional, Long, Arianna S., additional, Lotz, Jennifer M., additional, Lucas, Ray A., additional, Papovich, Casey, additional, Pentericci, Laura, additional, Pérez-González, Pablo G., additional, Pirzkal, Nor, additional, Rafelski, Marc, additional, Ravindranath, Swara, additional, Somerville, Rachel S., additional, Straughn, Amber N., additional, Tacchella, Sandro, additional, Trump, Jonathan R., additional, Wilkins, Stephen M., additional, Wuyts, Stijn, additional, Yung, L. Y. Aaron, additional, and Zavala, Jorge A., additional

Published
2023
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67. CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results

Author

Bagley, Micaela B., primary, Finkelstein, Steven L., additional, Koekemoer, Anton M., additional, Ferguson, Henry C., additional, Arrabal Haro, Pablo, additional, Dickinson, Mark, additional, Kartaltepe, Jeyhan S., additional, Papovich, Casey, additional, Pérez-González, Pablo G., additional, Pirzkal, Nor, additional, Somerville, Rachel S., additional, Willmer, Christopher N. A., additional, Yang, Guang, additional, Yung, L. Y. Aaron, additional, Fontana, Adriano, additional, Grazian, Andrea, additional, Grogin, Norman A., additional, Hirschmann, Michaela, additional, Kewley, Lisa J., additional, Kirkpatrick, Allison, additional, Kocevski, Dale D., additional, Lotz, Jennifer M., additional, Medrano, Aubrey, additional, Morales, Alexa M., additional, Pentericci, Laura, additional, Ravindranath, Swara, additional, Trump, Jonathan R., additional, Wilkins, Stephen M., additional, Calabrò, Antonello, additional, Cooper, M. C., additional, Costantin, Luca, additional, de la Vega, Alexander, additional, Hilbert, Bryan, additional, Hutchison, Taylor A., additional, Larson, Rebecca L., additional, Lucas, Ray A., additional, McGrath, Elizabeth J., additional, Ryan, Russell, additional, Wang, Xin, additional, and Wuyts, Stijn, additional

Published
2023
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68. Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations

Author

Zavala, Jorge A., primary, Buat, Véronique, additional, Casey, Caitlin M., additional, Finkelstein, Steven L., additional, Burgarella, Denis, additional, Bagley, Micaela B., additional, Ciesla, Laure, additional, Daddi, Emanuele, additional, Dickinson, Mark, additional, Ferguson, Henry C., additional, Franco, Maximilien, additional, Jiménez-Andrade, E. F., additional, Kartaltepe, Jeyhan S., additional, Koekemoer, Anton M., additional, Bail, Aurélien Le, additional, Murphy, E. J., additional, Papovich, Casey, additional, Tacchella, Sandro, additional, Wilkins, Stephen M., additional, Aretxaga, Itziar, additional, Behroozi, Peter, additional, Champagne, Jaclyn B., additional, Fontana, Adriano, additional, Giavalisco, Mauro, additional, Grazian, Andrea, additional, Grogin, Norman A., additional, Kewley, Lisa J., additional, Kocevski, Dale D., additional, Kirkpatrick, Allison, additional, Lotz, Jennifer M., additional, Pentericci, Laura, additional, Pérez-González, Pablo G., additional, Pirzkal, Nor, additional, Ravindranath, Swara, additional, Somerville, Rachel S., additional, Trump, Jonathan R., additional, Yang, Guang, additional, Yung, L. Y. Aaron, additional, Almaini, Omar, additional, Amorín, Ricardo O., additional, Annunziatella, Marianna, additional, Haro, Pablo Arrabal, additional, Backhaus, Bren E., additional, Barro, Guillermo, additional, Bell, Eric F., additional, Bhatawdekar, Rachana, additional, Bisigello, Laura, additional, Buitrago, Fernando, additional, Calabrò, Antonello, additional, Castellano, Marco, additional, Chávez Ortiz, Óscar A., additional, Chworowsky, Katherine, additional, Cleri, Nikko J., additional, Cohen, Seth H., additional, Cole, Justin W., additional, Cooke, Kevin C., additional, Cooper, M. C., additional, Cooray, Asantha R., additional, Costantin, Luca, additional, Cox, Isabella G., additional, Croton, Darren, additional, Davé, Romeel, additional, de la Vega, Alexander, additional, Dekel, Avishai, additional, Elbaz, David, additional, Estrada-Carpenter, Vicente, additional, Fernández, Vital, additional, Finkelstein, Keely D., additional, Freundlich, Jonathan, additional, Fujimoto, Seiji, additional, García-Argumánez, Ángela, additional, Gardner, Jonathan P., additional, Gawiser, Eric, additional, Gómez-Guijarro, Carlos, additional, Guo, Yuchen, additional, Hamilton, Timothy S., additional, Hathi, Nimish P., additional, Holwerda, Benne W., additional, Hirschmann, Michaela, additional, Huertas-Company, Marc, additional, Hutchison, Taylor A., additional, Iyer, Kartheik G., additional, Jaskot, Anne E., additional, Jha, Saurabh W., additional, Jogee, Shardha, additional, Juneau, Stéphanie, additional, Jung, Intae, additional, Kassin, Susan A., additional, Kurczynski, Peter, additional, Larson, Rebecca L., additional, Leung, Gene C. K., additional, Long, Arianna S., additional, Lucas, Ray A., additional, Magnelli, Benjamin, additional, Mantha, Kameswara Bharadwaj, additional, Matharu, Jasleen, additional, McGrath, Elizabeth J., additional, McIntosh, Daniel H., additional, Medrano, Aubrey, additional, Merlin, Emiliano, additional, Mobasher, Bahram, additional, Morales, Alexa M., additional, Newman, Jeffrey A., additional, Nicholls, David C., additional, Pandya, Viraj, additional, Rafelski, Marc, additional, Ronayne, Kaila, additional, Rose, Caitlin, additional, Ryan, Russell E., additional, Santini, Paola, additional, Seillé, Lise-Marie, additional, Shah, Ekta A., additional, Shen, Lu, additional, Simons, Raymond C., additional, Snyder, Gregory F., additional, Stanway, Elizabeth R., additional, Straughn, Amber N., additional, Teplitz, Harry I., additional, Vanderhoof, Brittany N., additional, Vega-Ferrero, Jesús, additional, Wang, Weichen, additional, Weiner, Benjamin J., additional, Willmer, Christopher N. A., additional, and Wuyts, Stijn, additional

Published
2023
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69. Extending the evolution of the stellar mass–size relation at z ≤ 2 to low stellar mass galaxies from HFF and CANDELS

Author

Nedkova, Kalina V, Häußler, Boris, Marchesini, Danilo, Dimauro, Paola, Brammer, Gabriel, Eigenthaler, Paul, Feinstein, Adina D, Ferguson, Henry C, Huertas-Company, Marc, Johnston, Evelyn J, Kado-Fong, Erin, Kartaltepe, Jeyhan S, Labbé, Ivo, Lange-Vagle, Daniel, Martis, Nicholas S, McGrath, Elizabeth J, Muzzin, Adam, Oesch, Pascal, Ordenes-Briceño, Yasna, Puzia, Thomas, Shipley, Heath V, Simmons, Brooke D, Skelton, Rosalind E, Stefanon, Mauro, van der Wel, Arjen, Whitaker, Katherine E, Nedkova, Kalina V, Häußler, Boris, Marchesini, Danilo, Dimauro, Paola, Brammer, Gabriel, Eigenthaler, Paul, Feinstein, Adina D, Ferguson, Henry C, Huertas-Company, Marc, Johnston, Evelyn J, Kado-Fong, Erin, Kartaltepe, Jeyhan S, Labbé, Ivo, Lange-Vagle, Daniel, Martis, Nicholas S, McGrath, Elizabeth J, Muzzin, Adam, Oesch, Pascal, Ordenes-Briceño, Yasna, Puzia, Thomas, Shipley, Heath V, Simmons, Brooke D, Skelton, Rosalind E, Stefanon, Mauro, van der Wel, Arjen, and Whitaker, Katherine E

Abstract

We reliably extend the stellar mass–size relation over 0.2 ≤ z ≤ 2 to low stellar mass galaxies by combining the depth of Hubble Frontier Fields with the large volume covered by CANDELS. Galaxies are simultaneously modelled in multiple bands using the tools developed by the MegaMorph project, allowing robust size (i.e. half-light radius) estimates even for small, faint, and high redshift galaxies. We show that above 107 M⊙, star-forming galaxies are well represented by a single power law on the mass–size plane over our entire redshift range. Conversely, the stellar mass–size relation is steep for quiescent galaxies with stellar masses $\ge 10^{10.3}\, {\rm M}_\odot$ and flattens at lower masses, regardless of whether quiescence is selected based on star-formation activity, rest-frame colours, or structural characteristics. This flattening occurs at sizes of ∼1 kpc at z ≤ 1. As a result, a double power law is preferred for the stellar mass–size relation of quiescent galaxies, at least above 10$^7\, {\rm M}_\odot$. We find no strong redshift dependence in the slope of the relation of star-forming galaxies as well as of high mass quiescent galaxies. We also show that star-forming galaxies with stellar masses $\ge 10^{9.5}\, {\rm M}_\odot$ and quiescent galaxies with stellar masses $\ge 10^{10.3}\, {\rm M}_\odot$ have undergone significant size growth since z ∼ 2, as expected; however, low mass galaxies have not. Finally, we supplement our data with predominantly quiescent dwarf galaxies from the core of the Fornax cluster, showing that the stellar mass–size relation is continuous below 10$^7\, {\rm M}_\odot$, but a more complicated functional form is necessary to describe the relation.

Published
2021

70. Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS

Author

Nedkova, Kalina, Haussler, Boris, Marchesini, Danilo, Dimauro, Paola, Brammer, Gabriel, Eigenthaler, Paul, Feinstein, Adina D., Ferguson, Henry C., Huertas-Company, Marc, Johnston, Evelyn J., Kado-Fong, Erin, Kartaltepe, Jeyhan S., Labbe, Ivo, Lange-Vagle, Daniel, Martis, Nicholas S., McGrath, Elizabeth J., Muzzin, Adam, Oesch, Pascal, Ordenes-Briceno, Yasna, Puzia, Thomas, Shipley, Heath, Simmons, Brooke D., Skelton, Rosalind E., Stefanon, Mauro, van der Wel, Arjen, Whitaker, Katherine E., Nedkova, Kalina, Haussler, Boris, Marchesini, Danilo, Dimauro, Paola, Brammer, Gabriel, Eigenthaler, Paul, Feinstein, Adina D., Ferguson, Henry C., Huertas-Company, Marc, Johnston, Evelyn J., Kado-Fong, Erin, Kartaltepe, Jeyhan S., Labbe, Ivo, Lange-Vagle, Daniel, Martis, Nicholas S., McGrath, Elizabeth J., Muzzin, Adam, Oesch, Pascal, Ordenes-Briceno, Yasna, Puzia, Thomas, Shipley, Heath, Simmons, Brooke D., Skelton, Rosalind E., Stefanon, Mauro, van der Wel, Arjen, and Whitaker, Katherine E.

Abstract

We reliably extend the stellar mass-size relation over 0.2 = 10(10.3)M(circle dot) and flattens at lower masses, regardless of whether quiescence is selected based on star-formation activity, rest-frame colours, or structural characteristics. This flattening occurs at sizes of similar to 1 kpc at z = 10(9.5)M(circle dot) and quiescent galaxies with stellar masses >= 10(10.3)M(circle dot) have undergone significant size growth since z similar to 2, as expected; however, low mass galaxies have not. Finally, we supplement our data with predominantly quiescent dwarf galaxies from the core of the Fornax cluster, showing that the stellar mass-size relation is continuous below 10(7)M(circle dot), but a more complicated functional form is necessary to describe the relation.

Published
2021

71. Extending the evolution of the stellar mass–size relation at z ≤ 2 to low stellar mass galaxies from HFF and CANDELS

Author

Nedkova, Kalina V, primary, Häußler, Boris, additional, Marchesini, Danilo, additional, Dimauro, Paola, additional, Brammer, Gabriel, additional, Eigenthaler, Paul, additional, Feinstein, Adina D, additional, Ferguson, Henry C, additional, Huertas-Company, Marc, additional, Johnston, Evelyn J, additional, Kado-Fong, Erin, additional, Kartaltepe, Jeyhan S, additional, Labbé, Ivo, additional, Lange-Vagle, Daniel, additional, Martis, Nicholas S, additional, McGrath, Elizabeth J, additional, Muzzin, Adam, additional, Oesch, Pascal, additional, Ordenes-Briceño, Yasna, additional, Puzia, Thomas, additional, Shipley, Heath V, additional, Simmons, Brooke D, additional, Skelton, Rosalind E, additional, Stefanon, Mauro, additional, van der Wel, Arjen, additional, and Whitaker, Katherine E, additional

Published
2021
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72. Investigating the Effect of Galaxy Interactions on the Enhancement of Active Galactic Nuclei at 0.5 < z < 3.0

Author

Shah, Ekta A., primary, Kartaltepe, Jeyhan S., additional, Magagnoli, Christina T., additional, Cox, Isabella G., additional, Wetherell, Caleb T., additional, Vanderhoof, Brittany N., additional, Calabro, Antonello, additional, Chartab, Nima, additional, Conselice, Christopher J., additional, Croton, Darren J., additional, Donley, Jennifer, additional, Groot, Laura de, additional, de la Vega, Alexander, additional, Hathi, Nimish P., additional, Ilbert, Olivier, additional, Inami, Hanae, additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Lemaux, Brian C., additional, Mantha, Kameswara Bharadwaj, additional, Marchesi, Stefano, additional, Martig, Marie, additional, Masters, Daniel C., additional, McGrath, Elizabeth J., additional, McIntosh, Daniel H., additional, Moreno, Jorge, additional, Nayyeri, Hooshang, additional, Pampliega, Belen Alcalde, additional, Salvato, Mara, additional, Snyder, Gregory F., additional, Straughn, Amber N., additional, Treister, Ezequiel, additional, and Weston, Madalyn E., additional

Published
2020
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73. Virtual monitoring of suicide risk in the general hospital and emergency department

Author

Kroll, David S., primary, Stanghellini, Escel, additional, DesRoches, Stephanie L., additional, Lydon, Charles, additional, Webster, Allison, additional, O'Reilly, Molly, additional, Hurwitz, Shelley, additional, Aylward, Patricia M., additional, Cartright, Jennifer A., additional, McGrath, Elizabeth J., additional, Delaporta, Linda, additional, Meyer, Anna T., additional, Kristan, Michael S., additional, Falaro, Laurie J., additional, Murphy, Colin, additional, Karno, Jennifer, additional, Pallin, Daniel J., additional, Schaffer, Adam, additional, Shah, Sejal B., additional, Lakatos, Barbara E., additional, Mitchell, Monique T., additional, Murphy, Christine A., additional, Gorman, Janet M., additional, Gitlin, David F., additional, and Mulloy, Deborah F., additional

Published
2020
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74. What Turns Galaxies Off? the Different Morphologies of Star-Forming and Quiescent Galaxies Since z Approximates 2 from CANDELS

Author

Bell, Eric F, VanDerWel, Arjen, Papovich, Casey, Kocevski, Dale, Lotz, Jennifer, McIntosh, Daniel H, Kartaltepe, Jeyhan, Faber, S. M, Ferguson, Harry, Koekemoer, Anton, Grogin, Norman, Wuyts, Stijn, Cheung, Edmong, Conselice, Christopher J, Dunlop, James S, Giavalisco, Mauro, Herrington, Jessica, Koo, David, McGrath, Elizabeth J, DeMello, Duilia, Rix, Hans-Walter, Robaina, Aday R, and Williams, Christina C

Subjects
Astrophysics
Abstract

We use HST/WFC3 imaging from the CANDELS multicyc1e treasury survey, in conjunction with the Sloan Digital Sky Survey, to explore the evolution of galactic structure for galaxies with stellar masses > 3 x 10(exp 10) Solar Mass from Z= 2.2 to the present epoch, a time span of 10 Gyr. We explore the relationship between rest-frame optical color, stellar mass, star formation activity and the structural parameters of galaxies as determined from parametric fits to the surface brightness profiles of galaxies. We confirm the dramatic evolution from z= 2.2 to the present day in the number density of non-star-forming galaxies above 3 x 10(exp 10) Solar Mass reported by other authors. We find that the vast majority of these quiescent systems have concentrated light profiles, as parameterized by the Sersic index, and the population of concentrated galaxies grows similarly rapidly. We examine the joint distribution of star formation activity, Sersic index, stellar mass, mass divided by radius (a proxy for velocity dispersion), and stellar surface density. Quiescence correlates poorly with stellar mass at all z < 2.2 (given the approx < 0.2 dex scatter between halo mass and stellar mass at z approximates 0 inferred by More et al, this argues against halo mass being the only factor determining quiescence). Quiescence correlates better with Sersic index, 'velocity dispersion' and stellar surface density, where Sersic index correlates the best (increasingly so at lower redshift). Yet, there is significant scatter between quiescence and galaxy structure: while the vast majority of quiescent galaxies have prominent bulges, many of them have significant disks, and a number of bulge-dominated galaxies have significant star formation. Noting the rarity of quiescent galaxies without prominent bulges, we argue that a prominent bulge (and, perhaps by association, a supermassive black hole) is a necessary but not sufficient condition for quenching star formation on galactic scales over the last 10 Gyr; such a result is qualitatively consistent with the expectations of the AGN feedback paradigm.

Published
2011

75. A CANDELS WFC3 Grism Study of Emission-Line Galaxies at Z approximates 2: A mix of Nuclear Activity and Low-Metallicity Star Formation

Author

Trump, Jonathan R, Weiner, Benjamin J, Scarlata, Claudia, Kocevski, Dale D, Bell, Eric F, McGrath, Elizabeth J, Koo, David C, Faber, S. M, Laird, Elise S, Mozena, Mark, Rangel, Cyprian, Yan, Renbin, Yesuf, Hassen, Atek, Hakim, Dickinson, Mark, Donley, Jennifer L, Dunlop, James S, Ferguson, Henry C, Finkelstein, Steven L, Grogin, Norman A, Hathi, Nimish P, Juneau, Stephanie, Kartaltepe, Jeyhan S, Koekemoer, Anton M, and Nandra, Kirpal

Subjects
Astrophysics
Abstract

We present Hubble Space Telescope Wide Field Camera 3 slitless grism spectroscopy of 28 emission-line galaxies at z approximates 2, in the GOODS-S region of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). The high sensitivity of these grism observations, with > 5-sigma detections of emission lines to f > 2.5 X 10(exp -18( erg/s/ square cm, means that the galaxies in the sample are typically approximately 7 times less massive (median M(star). = 10(exp 9.5)M(solar)) than previously studied z approximates 2 emission-line galaxies. Despite their lower mass, the galaxies have [O-III]/H-Beta ratios which are very similar to previously studied z approximates 2 galaxies and much higher than the typical emission-line ratios of local galaxies. The WFC3 grism allows for unique studies of spatial gradients in emission lines, and we stack the two-dimensional spectra of the galaxies for this purpose. In the stacked data the [O-III] emission line is more spatially concentrated than the H-Beta emission line with 98.1% confidence. We additionally stack the X-ray data (all sources are individually undetected), and find that the average L(sub [O-III])/L(sub 0.5.10keV) ratio is intermediate between typical z approximates 0 obscured active galaxies and star-forming galaxies. Together the compactness of the stacked [O-III] spatial profile and the stacked X-ray data suggest that at least some of these low-mass, low-metallicity galaxies harbor weak active galactic nuclei.

Published
2011

76. The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates

Author

Barro, Guillermo, primary, Pérez-González, Pablo G., additional, Cava, Antonio, additional, Brammer, Gabriel, additional, Pandya, Viraj, additional, Moral, Carmen Eliche, additional, Esquej, Pilar, additional, Domínguez-Sánchez, Helena, additional, Pampliega, Belen Alcalde, additional, Guo, Yicheng, additional, Koekemoer, Anton M., additional, Trump, Jonathan R., additional, Ashby, Matthew L. N., additional, Cardiel, Nicolas, additional, Castellano, Marco, additional, Conselice, Christopher J., additional, Dickinson, Mark E., additional, Dolch, Timothy, additional, Donley, Jennifer L., additional, Briones, Néstor Espino, additional, Faber, Sandra M., additional, Fazio, Giovanni G., additional, Ferguson, Henry, additional, Finkelstein, Steve, additional, Fontana, Adriano, additional, Galametz, Audrey, additional, Gardner, Jonathan P., additional, Gawiser, Eric, additional, Giavalisco, Mauro, additional, Grazian, Andrea, additional, Grogin, Norman A., additional, Hathi, Nimish P., additional, Hemmati, Shoubaneh, additional, Hernán-Caballero, Antonio, additional, Kocevski, Dale, additional, Koo, David C., additional, Kodra, Dritan, additional, Lee, Kyoung-Soo, additional, Lin, Lihwai, additional, Lucas, Ray A., additional, Mobasher, Bahram, additional, McGrath, Elizabeth J., additional, Nandra, Kirpal, additional, Nayyeri, Hooshang, additional, Newman, Jeffrey A., additional, Pforr, Janine, additional, Peth, Michael, additional, Rafelski, Marc, additional, Rodríguez-Munoz, Lucia, additional, Salvato, Mara, additional, Stefanon, Mauro, additional, Wel, Arjen van der, additional, Willner, Steven P., additional, Wiklind, Tommy, additional, and Wuyts, Stijn, additional

Published
2019
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77. Studying the physical properties of tidal features – I. Extracting morphological substructure in CANDELS observations and VELA simulations

Author

Mantha, Kameswara Bharadwaj, primary, McIntosh, Daniel H, primary, Ciaschi, Cody P, primary, Evan, Rubyet, primary, Ferguson, Henry C, primary, Fries, Logan B, primary, Guo, Yicheng, primary, Koekemoer, Anton M, primary, Landry, Luther D, primary, McGrath, Elizabeth J, primary, Simons, Raymond C, primary, Snyder, Gregory F, primary, Thompson, Scott E, primary, Bell, Eric F, primary, Ceverino, Daniel, primary, Hathi, Nimish P, primary, Pacifici, Camilla, primary, Primack, Joel R, primary, Rafelski, Marc, primary, and Rodriguez-Gomez, Vicente, primary

Published
2019
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78. CANDELS: Elevated black hole growth in the progenitors of compact quiescent galaxies at z ? 2

Author

Kocevski, Dale D., Barro, Guillermo, Faber, S.M., Dekel, Avishai, Somerville, Rachel S., Young, Joshua A., Williams, Christina C., McIntosh, Daniel H., Georgakakis, Antonis, Hasinger, Guenther, Nandra, Kirpal, Civano, Francesca, Alexander, David M., Almaini, Omar, Conselice, Christopher J., Donley, Jennifer L., Ferguson, Harry C., Giavalisco, Mauro, Grogin, Norman A., Hathi, Nimish, Hawkins, Matthew, Koekemoer, Anton M., Koo, David C., McGrath, Elizabeth J., Mobasher, Bahram, Pforr, Janine, Primack, Joel R., Santini, Paola, Stefanon, Mauro, Trump, Jonathan R., van der Wel, Arjen, Wuyts, Stijn, and Yan, Haojing

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We examine the fraction of massive (M* > 1010 M) compact star-forming galaxies (cSFGs) that host an active galactic nucleus (AGN) at z ~ 2. These cSFGs are likely the direct progenitors of the compact quiescent galaxies observed at this epoch, which are the first population of passive galaxies to appear in large numbers in the early Universe. We identify cSFGs that host an AGN using a combination of Hubble WFC3 imaging and Chandra X-ray observations in four fields: the Chandra Deep Fields, the Extended Groth Strip, and the UKIDSS Ultra Deep Survey field. We find that - 39.2+ % 3.6 3.9 (65/166) of cSFGs at 1.4 < z < 3.0 host an X-ray detected AGN. This fraction is 3.2 times higher than the incidence of AGN in extended star-forming galaxies with similar masses at these redshifts. This difference is significant at the 6.2s level. Our results are consistent with models in which cSFGs are formed through a dissipative contraction that triggers a compact starburst and concurrent growth of the central black hole. We also discuss our findings in the context of cosmological galaxy evolution simulations that require feedback energy to rapidly quench cSFGs. We show that the AGN fraction peaks precisely where energy injection is needed to reproduce the decline in the number density of cSFGs with redshift. Our results suggest that the first abundant population of massive quenched galaxies emerged directly following a phase of elevated supermassive black hole growth and further hints at a possible connection between AGN and the rapid quenching of star formation in these galaxies.

Published
2017

79. Demographics of Star-forming Galaxies since z ∼ 2.5. I. The UVJ Diagram in CANDELS

Author

Fang, Jerome J., primary, Faber, S. M., additional, Koo, David C., additional, Rodríguez-Puebla, Aldo, additional, Guo, Yicheng, additional, Barro, Guillermo, additional, Behroozi, Peter, additional, Brammer, Gabriel, additional, Chen, Zhu, additional, Dekel, Avishai, additional, Ferguson, Henry C., additional, Gawiser, Eric, additional, Giavalisco, Mauro, additional, Kartaltepe, Jeyhan, additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, McGrath, Elizabeth J., additional, McIntosh, Daniel, additional, Newman, Jeffrey A., additional, Pacifici, Camilla, additional, Pandya, Viraj, additional, Pérez-González, Pablo G., additional, Primack, Joel R., additional, Salmon, Brett, additional, Trump, Jonathan R., additional, Weiner, Benjamin, additional, Willner, S. P., additional, Acquaviva, Viviana, additional, Dahlen, Tomas, additional, Finkelstein, Steven L., additional, Finlator, Kristian, additional, Fontana, Adriano, additional, Galametz, Audrey, additional, Grogin, Norman A., additional, Gruetzbauch, Ruth, additional, Johnson, Seth, additional, Mobasher, Bahram, additional, Papovich, Casey J., additional, Pforr, Janine, additional, Salvato, Mara, additional, Santini, P., additional, van der Wel, Arjen, additional, Wiklind, Tommy, additional, and Wuyts, Stijn, additional

Published
2018
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80. The Isophotal Structure of Star-forming Galaxies at 0.5 < 1.8 in CANDELS: Implications for the Evolution of Galaxy Structure

Author

Jiang, Dongfei, primary, Liu, F. S., additional, Zheng, Xianzhong, additional, Yesuf, Hassen M., additional, Koo, David C., additional, Faber, S. M., additional, Guo, Yicheng, additional, Koekemoer, Anton M., additional, Wang, Weichen, additional, Fang, Jerome J., additional, Barro, Guillermo, additional, Jia, Meng, additional, Tong, Wei, additional, Liu, Lu, additional, Meng, Xianmin, additional, Kocevski, Dale, additional, McGrath, Elizabeth J., additional, and Hathi, Nimish P., additional

Published
2018
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81. CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies atz∼ 2

Author

Kocevski, Dale D., primary, Barro, Guillermo, additional, Faber, S. M., additional, Dekel, Avishai, additional, Somerville, Rachel S., additional, Young, Joshua A., additional, Williams, Christina C., additional, McIntosh, Daniel H., additional, Georgakakis, Antonis, additional, Hasinger, Guenther, additional, Nandra, Kirpal, additional, Civano, Francesca, additional, Alexander, David M., additional, Almaini, Omar, additional, Conselice, Christopher J., additional, Donley, Jennifer L., additional, Ferguson, Harry C., additional, Giavalisco, Mauro, additional, Grogin, Norman A., additional, Hathi, Nimish, additional, Hawkins, Matthew, additional, Koekemoer, Anton M., additional, Koo, David C., additional, McGrath, Elizabeth J., additional, Mobasher, Bahram, additional, Pérez González, Pablo G., additional, Pforr, Janine, additional, Primack, Joel R., additional, Santini, Paola, additional, Stefanon, Mauro, additional, Trump, Jonathan R., additional, van der Wel, Arjen, additional, Wuyts, Stijn, additional, and Yan, Haojing, additional

Published
2017
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82. Hidden Starbursts and Active Galactic Nuclei at 0

Author

Lemaux, Brian C., Floc'h, Emeric Le, F��vre, Olivier Le, Ilbert, Olivier, Tresse, Laurence, Lubin, Lori M., Zamorani, Giovanni, Gal, Roy R., Ciliegi, Paolo, Cassata, Paolo, Kocevski, Dale D., McGrath, Elizabeth J., Bardelli, Sandro, Zucca, Elena, and Squires, Gordon K.

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We investigate of the properties of $\sim$2000 Herschel/SPIRE-selected galaxies from $00.5$), the highest $L_{TIR}$ galaxies in a given redshift bin are unobserved by SPIRE at subsequently lower redshifts, a trend linked to downsizing. In conjunction with other results, this evidence is used to argue for prevalent AGN-driven quenching in starburst galaxies across cosmic time., 39 pages, 19 figures, 6 tables, accepted to A&A. Updated version contains minor revisions and corrects a typo made in equation 5. All data used in the paper is now available online through CDS

Published
2013
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83. The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5

Author

Cheung, Edmond, Faber, S. M., Koo, David C., Dutton, Aaron A., Simard, Luc, McGrath, Elizabeth J., Huang, J. -S., Bell, Eric F., Dekel, Avishai, Fang, Jerome J., Salim, Samir, Barro, G., Bundy, K., Coil, A. L., Cooper, Michael C., Conselice, C. J., Davis, M., Dominguez, A., Kassin, Susan A., Kocevski, Dale D., Koekemoer, Anton M., Lin, Lihwai, Lotz, Jennifer M., Newman, J. A., Phillips, Andrew C., Rosario, D. J., Weiner, Benjamin J., and Willmer, C. N. A.

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

The shutdown of star formation in galaxies is generally termed `quenching'. Although quenching may occur through a variety of processes, the exact mechanism(s) that is in fact responsible for quenching is still in question. This paper addresses quenching by searching for traces of possible quenching processes through their effects on galaxy structural parameters such as surface stellar mass density and Sersic index (n). We analyze the rest-frame U-B color correlations versus these structural parameters using a sample of galaxies in the redshift range 0.5< z, 28 pages, 13 figures

Published
2012
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84. UVUDF: ULTRAVIOLET THROUGH NEAR-INFRARED CATALOG AND PHOTOMETRIC REDSHIFTS OF GALAXIES IN THE HUBBLE ULTRA DEEP FIELD

Author

Rafelski, Marc, primary, Teplitz, Harry I., additional, Gardner, Jonathan P., additional, Coe, Dan, additional, Bond, Nicholas A., additional, Koekemoer, Anton M., additional, Grogin, Norman, additional, Kurczynski, Peter, additional, McGrath, Elizabeth J., additional, Bourque, Matthew, additional, Atek, Hakim, additional, Brown, Thomas M., additional, Colbert, James W., additional, Codoreanu, Alex, additional, Ferguson, Henry C., additional, Finkelstein, Steven L., additional, Gawiser, Eric, additional, Giavalisco, Mauro, additional, Gronwall, Caryl, additional, Hanish, Daniel J., additional, Lee, Kyoung-Soo, additional, Mehta, Vihang, additional, de Mello, Duilia F., additional, Ravindranath, Swara, additional, Ryan, Russell E., additional, Scarlata, Claudia, additional, Siana, Brian, additional, Soto, Emmaris, additional, and Voyer, Elysse N., additional

Published
2015
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85. BULGE GROWTH AND QUENCHING SINCEz= 2.5 IN CANDELS/3D-HST

Author

Lang, Philipp, primary, Wuyts, Stijn, additional, Somerville, Rachel S., additional, Schreiber, Natascha M. Förster, additional, Genzel, Reinhard, additional, Bell, Eric F., additional, Brammer, Gabe, additional, Dekel, Avishai, additional, Faber, Sandra M., additional, Ferguson, Henry C., additional, Grogin, Norman A., additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Lutz, Dieter, additional, McGrath, Elizabeth J., additional, Momcheva, Ivelina, additional, Nelson, Erica J., additional, Primack, Joel R., additional, Rosario, David J., additional, Skelton, Rosalind E., additional, Tacconi, Linda J., additional, van Dokkum, Pieter G., additional, and Whitaker, Katherine E., additional

Published
2014
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86. PROPERTIES OF SUBMILLIMETER GALAXIES IN THE CANDELS GOODS-SOUTH FIELD

Author

Wiklind, Tommy, primary, Conselice, Christopher J., additional, Dahlen, Tomas, additional, Dickinson, Mark E., additional, Ferguson, Henry C., additional, Grogin, Norman A., additional, Guo, Yicheng, additional, Koekemoer, Anton M., additional, Mobasher, Bahram, additional, Mortlock, Alice, additional, Fontana, Adriano, additional, Davé, Romeel, additional, Yan, Haojing, additional, Acquaviva, Viviana, additional, Ashby, Matthew L. N., additional, Barro, Guillermo, additional, Caputi, Karina I., additional, Castellano, Marco, additional, Dekel, Avishai, additional, Donley, Jennifer L., additional, Fazio, Giovanni G., additional, Giavalisco, Mauro, additional, Grazian, Andrea, additional, Hathi, Nimish P., additional, Kurczynski, Peter, additional, Lu, Yu, additional, McGrath, Elizabeth J., additional, de Mello, Duilia F., additional, Peth, Michael, additional, Safarzadeh, Mohammad, additional, Stefanon, Mauro, additional, and Targett, Thomas, additional

Published
2014
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88. A CANDELS-3D-HST SYNERGY: RESOLVED STAR FORMATION PATTERNS AT 0.7 < 1.5

Author

Wuyts, Stijn, primary, Förster Schreiber, Natascha M., additional, Nelson, Erica J., additional, van Dokkum, Pieter G., additional, Brammer, Gabe, additional, Chang, Yu-Yen, additional, Faber, Sandra M., additional, Ferguson, Henry C., additional, Franx, Marijn, additional, Fumagalli, Mattia, additional, Genzel, Reinhard, additional, Grogin, Norman A., additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Lundgren, Britt, additional, Lutz, Dieter, additional, McGrath, Elizabeth J., additional, Momcheva, Ivelina, additional, Rosario, David, additional, Skelton, Rosalind E., additional, Tacconi, Linda J., additional, van der Wel, Arjen, additional, and Whitaker, Katherine E., additional

Published
2013
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89. A CRITICAL ASSESSMENT OF PHOTOMETRIC REDSHIFT METHODS: A CANDELS INVESTIGATION

Author

Dahlen, Tomas, primary, Mobasher, Bahram, additional, Faber, Sandra M., additional, Ferguson, Henry C., additional, Barro, Guillermo, additional, Finkelstein, Steven L., additional, Finlator, Kristian, additional, Fontana, Adriano, additional, Gruetzbauch, Ruth, additional, Johnson, Seth, additional, Pforr, Janine, additional, Salvato, Mara, additional, Wiklind, Tommy, additional, Wuyts, Stijn, additional, Acquaviva, Viviana, additional, Dickinson, Mark E., additional, Guo, Yicheng, additional, Huang, Jiasheng, additional, Huang, Kuang-Han, additional, Newman, Jeffrey A., additional, Bell, Eric F., additional, Conselice, Christopher J., additional, Galametz, Audrey, additional, Gawiser, Eric, additional, Giavalisco, Mauro, additional, Grogin, Norman A., additional, Hathi, Nimish, additional, Kocevski, Dale, additional, Koekemoer, Anton M., additional, Koo, David C., additional, Lee, Kyoung-Soo, additional, McGrath, Elizabeth J., additional, Papovich, Casey, additional, Peth, Michael, additional, Ryan, Russell, additional, Somerville, Rachel, additional, Weiner, Benjamin, additional, and Wilson, Grant, additional

Published
2013
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90. STRUCTURAL EVOLUTION OF EARLY-TYPE GALAXIES TOz= 2.5 IN CANDELS

Author

Chang, Yu-Yen, primary, van der Wel, Arjen, additional, Rix, Hans-Walter, additional, Holden, Bradford, additional, Bell, Eric F., additional, McGrath, Elizabeth J., additional, Wuyts, Stijn, additional, Häussler, Boris, additional, Barden, Marco, additional, Faber, S. M., additional, Mozena, Mark, additional, Ferguson, Henry C., additional, Guo, Yicheng, additional, Galametz, Audrey, additional, Grogin, Norman A., additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Dekel, Avishai, additional, Huang, Kuang-Han, additional, Hathi, Nimish P., additional, and Donley, Jennifer, additional

Published
2013
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91. CANDELS MULTI-WAVELENGTH CATALOGS: SOURCE DETECTION AND PHOTOMETRY IN THE GOODS-SOUTH FIELD

Author

Guo, Yicheng, primary, Ferguson, Henry C., additional, Giavalisco, Mauro, additional, Barro, Guillermo, additional, Willner, S. P., additional, Ashby, Matthew L. N., additional, Dahlen, Tomas, additional, Donley, Jennifer L., additional, Faber, Sandra M., additional, Fontana, Adriano, additional, Galametz, Audrey, additional, Grazian, Andrea, additional, Huang, Kuang-Han, additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Koo, David C., additional, McGrath, Elizabeth J., additional, Peth, Michael, additional, Salvato, Mara, additional, Wuyts, Stijn, additional, Castellano, Marco, additional, Cooray, Asantha R., additional, Dickinson, Mark E., additional, Dunlop, James S., additional, Fazio, G. G., additional, Gardner, Jonathan P., additional, Gawiser, Eric, additional, Grogin, Norman A., additional, Hathi, Nimish P., additional, Hsu, Li-Ting, additional, Lee, Kyoung-Soo, additional, Lucas, Ray A., additional, Mobasher, Bahram, additional, Nandra, Kirpal, additional, Newman, Jeffery A., additional, and van der Wel, Arjen, additional

Published
2013
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92. CANDELS OBSERVATIONS OF THE ENVIRONMENTAL DEPENDENCE OF THE COLOR-MASS-MORPHOLOGY RELATION ATz= 1.6

Author

Bassett, Robert, primary, Papovich, Casey, additional, Lotz, Jennifer M., additional, Bell, Eric F., additional, Finkelstein, Steven L., additional, Newman, Jeffrey A., additional, Tran, Kim-Vy, additional, Almaini, Omar, additional, Lani, Caterina, additional, Cooper, Michael, additional, Croton, Darren, additional, Dekel, Avishai, additional, Ferguson, Henry C., additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Koo, David C., additional, McGrath, Elizabeth J., additional, McIntosh, Daniel H., additional, and Wechsler, Risa, additional

Published
2013
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93. SERENDIPITOUS DISCOVERY OF A MASSIVE cD GALAXY ATz= 1.096: IMPLICATIONS FOR THE EARLY FORMATION AND LATE EVOLUTION OF cD GALAXIES

Author

Liu, F. S., primary, Guo, Yicheng, additional, Koo, David C., additional, Trump, Jonathan R., additional, Barro, Guillermo, additional, Yesuf, Hassen, additional, Faber, S. M., additional, Giavalisco, M., additional, Cassata, P., additional, Koekemoer, A. M., additional, Pentericci, L., additional, Castellano, M., additional, Cheung, Edmond, additional, Mao, Shude, additional, Xia, X. Y., additional, Grogin, Norman A., additional, Hathi, Nimish P., additional, Huang, Kuang-Han, additional, Kocevski, Dale, additional, McGrath, Elizabeth J., additional, and Wuyts, Stijn, additional

Published
2013
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94. CANDELS MULTIWAVELENGTH CATALOGS: SOURCE IDENTIFICATION AND PHOTOMETRY IN THE CANDELS UKIDSS ULTRA-DEEP SURVEY FIELD

Author

Galametz, Audrey, primary, Grazian, Andrea, additional, Fontana, Adriano, additional, Ferguson, Henry C., additional, Ashby, M. L. N., additional, Barro, Guillermo, additional, Castellano, Marco, additional, Dahlen, Tomas, additional, Donley, Jennifer L., additional, Faber, Sandy M., additional, Grogin, Norman, additional, Guo, Yicheng, additional, Huang, Kuang-Han, additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Lee, Kyoung-Soo, additional, McGrath, Elizabeth J., additional, Peth, Michael, additional, Willner, S. P., additional, Almaini, Omar, additional, Cooper, Michael, additional, Cooray, Asantha, additional, Conselice, Christopher J., additional, Dickinson, Mark, additional, Dunlop, James S., additional, Fazio, G. G., additional, Foucaud, Sebastien, additional, Gardner, Jonathan P., additional, Giavalisco, Mauro, additional, Hathi, N. P., additional, Hartley, Will G., additional, Koo, David C., additional, Lai, Kamson, additional, de Mello, Duilia F., additional, McLure, Ross J., additional, Lucas, Ray A., additional, Paris, Diego, additional, Pentericci, Laura, additional, Santini, Paola, additional, Simpson, Chris, additional, Sommariva, Veronica, additional, Targett, Thomas, additional, Weiner, Benjamin J., additional, and Wuyts, Stijn, additional

Published
2013
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95. THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ⩽z< 0.8 IN THE DEEP2/AEGIS SURVEY

Author

Cheung, Edmond, primary, Faber, S. M., additional, Koo, David C., additional, Dutton, Aaron A., additional, Simard, Luc, additional, McGrath, Elizabeth J., additional, Huang, J.-S., additional, Bell, Eric F., additional, Dekel, Avishai, additional, Fang, Jerome J., additional, Salim, Samir, additional, Barro, G., additional, Bundy, K., additional, Coil, A. L., additional, Cooper, Michael C., additional, Conselice, C. J., additional, Davis, M., additional, Domínguez, A., additional, Kassin, Susan A., additional, Kocevski, Dale D., additional, Koekemoer, Anton M., additional, Lin, Lihwai, additional, Lotz, Jennifer M., additional, Newman, J. A., additional, Phillips, Andrew C., additional, Rosario, D. J., additional, Weiner, Benjamin J., additional, and Willmer, C. N. A., additional

Published
2012
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96. WHAT TURNS GALAXIES OFF? THE DIFFERENT MORPHOLOGIES OF STAR-FORMING AND QUIESCENT GALAXIES SINCEz∼ 2 FROM CANDELS

Author

Bell, Eric F., primary, van der Wel, Arjen, additional, Papovich, Casey, additional, Kocevski, Dale, additional, Lotz, Jennifer, additional, McIntosh, Daniel H., additional, Kartaltepe, Jeyhan, additional, Faber, S. M., additional, Ferguson, Harry, additional, Koekemoer, Anton, additional, Grogin, Norman, additional, Wuyts, Stijn, additional, Cheung, Edmond, additional, Conselice, Christopher J., additional, Dekel, Avishai, additional, Dunlop, James S., additional, Giavalisco, Mauro, additional, Herrington, Jessica, additional, Koo, David C., additional, McGrath, Elizabeth J., additional, de Mello, Duilia, additional, Rix, Hans-Walter, additional, Robaina, Aday R., additional, and Williams, Christina C., additional

Published
2012
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97. CANDELS: CORRELATIONS OF SPECTRAL ENERGY DISTRIBUTIONS AND MORPHOLOGIES WITH STAR FORMATION STATUS FOR MASSIVE GALAXIES ATz∼ 2

Author

Wang, Tao, primary, Huang, Jia-Sheng, additional, Faber, S. M., additional, Fang, Guanwen, additional, Wuyts, Stijn, additional, Fazio, G. G., additional, Yan, Haojing, additional, Dekel, Avishai, additional, Guo, Yicheng, additional, Ferguson, Henry C., additional, Grogin, Norman, additional, Lotz, Jennifer M., additional, Weiner, Benjamin, additional, McGrath, Elizabeth J., additional, Kocevski, Dale, additional, Hathi, Nimish P., additional, Lucas, Ray A., additional, Koekemoer, A. M., additional, Kong, Xu, additional, and Gu, Qiu-Sheng, additional

Published
2012
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98. CANDELS: CONSTRAINING THE AGN-MERGER CONNECTION WITH HOST MORPHOLOGIES ATz∼ 2

Author

Kocevski, Dale D., primary, Faber, S. M., additional, Mozena, Mark, additional, Koekemoer, Anton M., additional, Nandra, Kirpal, additional, Rangel, Cyprian, additional, Laird, Elise S., additional, Brusa, Marcella, additional, Wuyts, Stijn, additional, Trump, Jonathan R., additional, Koo, David C., additional, Somerville, Rachel S., additional, Bell, Eric F., additional, Lotz, Jennifer M., additional, Alexander, David M., additional, Bournaud, Frederic, additional, Conselice, Christopher J., additional, Dahlen, Tomas, additional, Dekel, Avishai, additional, Donley, Jennifer L., additional, Dunlop, James S., additional, Finoguenov, Alexis, additional, Georgakakis, Antonis, additional, Giavalisco, Mauro, additional, Guo, Yicheng, additional, Grogin, Norman A., additional, Hathi, Nimish P., additional, Juneau, Stéphanie, additional, Kartaltepe, Jeyhan S., additional, Lucas, Ray A., additional, McGrath, Elizabeth J., additional, McIntosh, Daniel H., additional, Mobasher, Bahram, additional, Robaina, Aday R., additional, Rosario, David, additional, Straughn, Amber N., additional, van der Wel, Arjen, additional, and Villforth, Carolin, additional

Published
2011
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99. A CANDELS WFC3 GRISM STUDY OF EMISSION-LINE GALAXIES ATz∼ 2: A MIX OF NUCLEAR ACTIVITY AND LOW-METALLICITY STAR FORMATION

Author

Trump, Jonathan R., primary, Weiner, Benjamin J., additional, Scarlata, Claudia, additional, Kocevski, Dale D., additional, Bell, Eric F., additional, McGrath, Elizabeth J., additional, Koo, David C., additional, Faber, S. M., additional, Laird, Elise S., additional, Mozena, Mark, additional, Rangel, Cyprian, additional, Yan, Renbin, additional, Yesuf, Hassen, additional, Atek, Hakim, additional, Dickinson, Mark, additional, Donley, Jennifer L., additional, Dunlop, James S., additional, Ferguson, Henry C., additional, Finkelstein, Steven L., additional, Grogin, Norman A., additional, Hathi, Nimish P., additional, Juneau, Stéphanie, additional, Kartaltepe, Jeyhan S., additional, Koekemoer, Anton M., additional, Nandra, Kirpal, additional, Newman, Jeffrey A., additional, Rodney, Steven A., additional, Straughn, Amber N., additional, and Teplitz, Harry I., additional

Published
2011
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100. CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY—THE HUBBLE SPACE TELESCOPE OBSERVATIONS, IMAGING DATA PRODUCTS, AND MOSAICS

Author

Koekemoer, Anton M., primary, Faber, S. M., additional, Ferguson, Henry C., additional, Grogin, Norman A., additional, Kocevski, Dale D., additional, Koo, David C., additional, Lai, Kamson, additional, Lotz, Jennifer M., additional, Lucas, Ray A., additional, McGrath, Elizabeth J., additional, Ogaz, Sara, additional, Rajan, Abhijith, additional, Riess, Adam G., additional, Rodney, Steve A., additional, Strolger, Louis, additional, Casertano, Stefano, additional, Castellano, Marco, additional, Dahlen, Tomas, additional, Dickinson, Mark, additional, Dolch, Timothy, additional, Fontana, Adriano, additional, Giavalisco, Mauro, additional, Grazian, Andrea, additional, Guo, Yicheng, additional, Hathi, Nimish P., additional, Huang, Kuang-Han, additional, van der Wel, Arjen, additional, Yan, Hao-Jing, additional, Acquaviva, Viviana, additional, Alexander, David M., additional, Almaini, Omar, additional, Ashby, Matthew L. N., additional, Barden, Marco, additional, Bell, Eric F., additional, Bournaud, Frédéric, additional, Brown, Thomas M., additional, Caputi, Karina I., additional, Cassata, Paolo, additional, Challis, Peter J., additional, Chary, Ranga-Ram, additional, Cheung, Edmond, additional, Cirasuolo, Michele, additional, Conselice, Christopher J., additional, Cooray, Asantha Roshan, additional, Croton, Darren J., additional, Daddi, Emanuele, additional, Davé, Romeel, additional, de Mello, Duilia F., additional, de Ravel, Loic, additional, Dekel, Avishai, additional, Donley, Jennifer L., additional, Dunlop, James S., additional, Dutton, Aaron A., additional, Elbaz, David, additional, Fazio, Giovanni G., additional, Filippenko, Alexei V., additional, Finkelstein, Steven L., additional, Frazer, Chris, additional, Gardner, Jonathan P., additional, Garnavich, Peter M., additional, Gawiser, Eric, additional, Gruetzbauch, Ruth, additional, Hartley, Will G., additional, Häussler, Boris, additional, Herrington, Jessica, additional, Hopkins, Philip F., additional, Huang, Jia-Sheng, additional, Jha, Saurabh W., additional, Johnson, Andrew, additional, Kartaltepe, Jeyhan S., additional, Khostovan, Ali A., additional, Kirshner, Robert P., additional, Lani, Caterina, additional, Lee, Kyoung-Soo, additional, Li, Weidong, additional, Madau, Piero, additional, McCarthy, Patrick J., additional, McIntosh, Daniel H., additional, McLure, Ross J., additional, McPartland, Conor, additional, Mobasher, Bahram, additional, Moreira, Heidi, additional, Mortlock, Alice, additional, Moustakas, Leonidas A., additional, Mozena, Mark, additional, Nandra, Kirpal, additional, Newman, Jeffrey A., additional, Nielsen, Jennifer L., additional, Niemi, Sami, additional, Noeske, Kai G., additional, Papovich, Casey J., additional, Pentericci, Laura, additional, Pope, Alexandra, additional, Primack, Joel R., additional, Ravindranath, Swara, additional, Reddy, Naveen A., additional, Renzini, Alvio, additional, Rix, Hans-Walter, additional, Robaina, Aday R., additional, Rosario, David J., additional, Rosati, Piero, additional, Salimbeni, Sara, additional, Scarlata, Claudia, additional, Siana, Brian, additional, Simard, Luc, additional, Smidt, Joseph, additional, Snyder, Diana, additional, Somerville, Rachel S., additional, Spinrad, Hyron, additional, Straughn, Amber N., additional, Telford, Olivia, additional, Teplitz, Harry I., additional, Trump, Jonathan R., additional, Vargas, Carlos, additional, Villforth, Carolin, additional, Wagner, Cory R., additional, Wandro, Pat, additional, Wechsler, Risa H., additional, Weiner, Benjamin J., additional, Wiklind, Tommy, additional, Wild, Vivienne, additional, Wilson, Grant, additional, Wuyts, Stijn, additional, and Yun, Min S., additional

Published
2011
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