572 citations · 9.7k across the 104 of their papers we have counts for
105 papers
Cosmic Collisions I: Optical Morphologies for MIRI-selected galaxies from the PRIMER survey
Gregory Troiani, Allison Kirkpatrick, Leyna Bajaj +7
We present the first results of visual morphology classifications from the Cosmic Collisions project, comprising 14,657 galaxies from the JWST Public Release IMaging for Extragalac…
Quiescent Galaxies at from CAPERS spectroscopy and their Number densities
Lu Shen, Weida Hu, Casey Papovich +28
Recent JWST observations have revealed an overabundance of quiescent galaxies at high redshift. Photometric methods, such as photometry-derived sSFRs, colors, and synthetic $…
The JWST Emission Line Survey (JELS): Multi-wavelength properties of Paschen line-emitters at Cosmic Noon
Malte Brinch, Edo Ibar, Luis Ossa-Fuentes +14
Context: Narrowband JWST/NIRCam selection isolates star-forming galaxies in well-defined redshift slices, while ALMA and archival far-IR/submm data reveal obscured growth. We combi…
A large population of strongly lensed faint submillimetre galaxies in future dark energy surveys inferred from JWST imaging
James Pearson, Stephen Serjeant, Wei-Hao Wang +13
Bright galaxies at sub-millimetre wavelengths from Herschel are now well known to be predominantly strongly gravitationally lensed. The same models that successfully predicted this…
Extended H over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at
Chian-Chou Chen, C. M. Harrison, I. Smail +15
Using data from ALMA and near-infrared (NIR) integral field spectrographs including both SINFONI and KMOS on the VLT, we investigate the two-dimensional distributions of H and r…
How to Measure Galaxy Star Formation Histories II: Nonparametric Models
Joel Leja, Adam C. Carnall, Benjamin D. Johnson +2
Nonparametric star formation histories (SFHs) have long promised to be the `gold standard' for galaxy spectral energy distribution (SED) modeling as they are flexible enough to des…