350 citations · 1.3k across the 18 of their papers we have counts for
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Improved SED-Fitting Assumptions Result in Inside-Out Quenching at and Quenching at All Radii Simultaneously at
Alexander de la Vega, Susan A. Kassin, Camilla Pacifici +6
Many studies conclude that galaxies quench from the inside-out by examining profiles of specific star-formation rate (sSFR). These are usually measured by fitting spectral energy d…
The Cosmic Evolution Early Release Science Survey (CEERS)
Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro +96
We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hour Director's Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates e…
SDSS-IV MaNGA: Stellar rotational support in disk galaxies vs. central surface density and stellar population age
Xiaohan Wang, Yifei Luo, S. M. Faber +10
We investigate how the stellar rotational support changes as a function of spatially resolved stellar population age () and relative central stellar surface density ($…
The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
Camilla Pacifici, Kartheik G. Iyer, Bahram Mobasher +52
The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy…
CEERS Key Paper V: A triality on the nature of HST-dark galaxies
Pablo G. Pérez-González, Guillermo Barro, Marianna Annunziatella +52
The new capabilities that JWST offers in the near- and mid-infrared (IR) are used to investigate in unprecedented detail the nature of optical/near-IR faint, mid-IR bright sources,…
First Look at z > 1 Bars in the Rest-Frame Near-Infrared with JWST Early CEERS Imaging
Yuchen Guo, Shardha Jogee, Steven L. Finkelstein +45
Stellar bars are key drivers of secular evolution in galaxies and can be effectively studied using rest-frame near-infrared (NIR) images, which trace the underlying stellar mass an…
Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations
Jorge A. Zavala, Veronique Buat, Caitlin M. Casey +121
Lyman Break Galaxy (LBG) candidates at z>10 are rapidly being identified in JWST/NIRCam observations. Due to the (redshifted) break produced by neutral hydrogen absorption of rest-…
A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging
Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro +117
We report the discovery of a candidate galaxy with a photo-z of z~12 in the first epoch of the JWST Cosmic Evolution Early Release Science (CEERS) Survey. Following conservative se…
The Dwarf Galaxy Population at : A Catalog of Emission Lines and Redshifts from Deep Keck Observations
John Pharo, Yicheng Guo, Guillermo Barro Calvo +18
We present a catalog of spectroscopically measured redshifts over and emission line fluxes for 1440 galaxies. The majority (65\%) of the galaxies come from the HA…
The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3
Weichen Wang, Susan A. Kassin, S. M. Faber +12
Strong galactic winds are ubiquitous at . However, it is not well known where inside galaxies these winds are launched from. We study the cool winds (\,K) in…
Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
Raymond C. Simons, Susan A. Kassin, Gregory F. Snyder +9
The majority of massive star-forming galaxies at have velocity gradients suggestive of rotation, in addition to large amounts of disordered motions. In this paper, we demo…
Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts
Weichen Wang, Susan A. Kassin, Camilla Pacifici +11
At intermediate and high redshifts, measurements of galaxy star-formation rates are usually based on rest-frame ultraviolet (UV) data. A correction for dust attenuation, A_UV, is n…
On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELS
F. S. Liu, Meng Jia, Hassen M. Yesuf +19
We investigate the galaxy quenching process at intermediate redshift using a sample of galaxies with between redshift 0.5 and 1.0 in all fiv…
The Isophotal Structure of Star-forming Galaxies at in CANDELS: Implications for the Evolution of Galaxy Structure
Dongfei Jiang, F. S. Liu, Xianzhong Zheng +15
We have measured the radial profiles of isophotal ellipticity () and disky/boxy parameter A out to radii of about three times the semi-major axes for s…
Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at
Yicheng Guo, Marc Rafelski, Eric F. Bell +20
Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists have not reached a co…
The Origins of UV-optical Color Gradients in Star-forming Galaxies at z ~ 2: Predominant Dust Gradients But Negligible sSFR Gradients
F. S. Liu, Dongfei Jiang, S. M. Faber +13
The rest-frame UV-optical (i.e., ) color is sensitive to both low-level recent star formation (specific star formation rate - sSFR) and dust. In this Letter, we extend our p…
UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles
Weichen Wang, S. M. Faber, F. S. Liu +10
This paper uses radial colour profiles to infer the distributions of dust, gas and star formation in z=0.4-1.4 star-forming main sequence galaxies. We start with the standard UVJ-b…
The UV-optical Color Gradients in Star-Forming Galaxies at 0.5<z<1.5: Origins and Link to Galaxy Assembly
F. S. Liu, Dongfei Jiang, Yicheng Guo +10
The rest-frame UV-optical (i.e., NUV-B) color index is sensitive to the low-level recent star formation and dust extinction, but it is insensitive to the metallicity. In this Lette…