activity
20202023
most citedTemplates for Fitting Photometry of Ultra-High-Redshift Galaxies

85 citations · 278 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2023

A Value-added COSMOS2020 Catalog of Physical Properties: Constraining Temperature-dependent Initial Mass Function

Vadim Rusakov, Charles L. Steinhardt, Albert Sneppen

This work presents and releases a catalog of new photometrically-derived physical properties for the most well-measured galaxies in the COSMOS field on the sky. Using a…

astro-ph.HE2023★ 2 cited

A broad-line quasar with unexplained extreme velocity offsets: post-shock outflow?

V. Rusakov, C. L. Steinhardt, M. Schramm +4

The quasar SDSS 0956+5128 exhibits three distinct velocity components with large offsets in emission: the systemic velocity of [O II], [O III] and [Ne III] narrow lines have redshi…

astro-ph.HE2023★ 29 cited

Classification of BATSE, Swift, and Fermi Gamma-Ray Bursts from Prompt Emission Alone

Charles L. Steinhardt, William J. Mann, Vadim Rusakov +1

Although it is generally assumed that there are two dominant classes of gamma-ray bursts (GRB) with different typical durations, it has been difficult to unambiguously classify GRB…

astro-ph.GA2023★ 4 cited

The Earliest Stage of Galactic Star Formation

Charles L. Steinhardt, Vadim Rusakov, Thomas H. Clark +5

Using a recently-developed technique to estimate gas temperatures () in star-forming regions from large photometric surveys, we propose a diagram, analogous to the H…

astro-ph.GA2022★ 85 cited

Templates for Fitting Photometry of Ultra-High-Redshift Galaxies

Charles L. Steinhardt, Vasily Kokorev, Vadim Rusakov +2

Recent data from the James Webb Space Telescope allow a first glimpse of galaxies at . The most successful tool for identifying ultra-high-redshift candidates and inf…

astro-ph.GA2022★ 14 cited

Implications of a Temperature Dependent IMF III: Mass Growth and Quiescence

Charles L. Steinhardt, Albert Sneppen, Hagan Hensley +10

The stellar initial mass function (IMF) is predicted to depend upon the temperature of gas in star-forming molecular clouds. The introduction of an additional parameter, …