1.4k citations · 6k across the 28 of their papers we have counts for
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Stellar Populations With Optical Spectra: Deep Learning vs. Popular Spectrum Fitting Codes
Joanna Woo, Dan Walters, Finn Archinuk +4
We compare the performance of several popular spectrum fitting codes (Firefly, starlight, pyPipe3D and pPXF), and a deep-learning convolutional neural network (StarNet), in recover…
-M* Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR-M* Diagrams
Samir Salim, Sandro Tacchella, Chandler Osborne +3
The specific star formation rate (sSFR) is commonly used to describe the level of galaxy star formation (SF) and to select quenched galaxies. However, being a relative measure of t…
Galaxies Going Bananas: Inferring the 3D Geometry of High-Redshift Galaxies with JWST-CEERS
Viraj Pandya, Haowen Zhang, Marc Huertas-Company +53
The 3D geometry of high-redshift galaxies remains poorly understood. We build a differentiable Bayesian model and use Hamiltonian Monte Carlo to efficiently and robustly infer the…
Molecular Gas during the Post-Starburst Phase: Low Gas Fractions in Green Valley Seyfert Post-Starburst Galaxies
Hassen M. Yesuf, K. Decker French, S. M. Faber +1
Post-starbursts (PSBs) are candidate for rapidly transitioning from star-bursting to quiescent galaxies. We study the molecular gas evolution of PSBs at z ~ 0.03 - 0.2. We undertoo…
No evidence for feedback: Unexceptional Low-ionization winds in Host galaxies of Low Luminosity Active Galactic Nuclei at Redshift z ~1
Hassen M. Yesuf, David C. Koo, S. M. Faber +6
We study winds in 12 X-ray AGN host galaxies at z ~ 1. We find, using the low-ionization Fe II 2586 absorption in the stacked spectra, that the probability distribution function (P…
The Galaxy-Halo Connection Over The Last 13.3 Gyrs
Aldo Rodriguez-Puebla, Joel R. Primack, Vladimir Avila-Reese +1
We present new determinations of the stellar-to-halo mass relation (SHMR) at that match the evolution of the galaxy stellar mass function, the SFR relation,and the c…
The evolution of star formation histories of quiescent galaxies
Camilla Pacifici, Susan A. Kassin, Benjamin J. Weiner +22
Although there has been much progress in understanding how galaxies evolve, we still do not understand how and when they stop forming stars and become quiescent. We address this by…
3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since
A. van der Wel, M. Franx, P. G. van Dokkum +27
Spectroscopic + photometric redshifts, stellar mass estimates, and rest-frame colors from the 3D-HST survey are combined with structural parameter measurements from CANDELS imaging…