most citedStochastic star formation and the abundance of UV-bright galaxies

14 citations · 15 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

Effect of ionizing photon escape fraction in faint galaxies on modeling reionization history of the universe

Zewei Wu, Andrey Kravtsov, Harley Katz

We present model calculations of the reionization history of hydrogen using star formation histories, computed with a galaxy formation model which reproduces properties of local dw…

astro-ph.GA2025

On the connection between nitrogen-enhanced field stars and the Galactic globular clusters

Sarah G. Kane, Vasily Belokurov, Stephanie Monty +6

As sites of some of the most efficient star formation in the Universe, globular clusters (GCs) have long been hypothesized to be the building blocks of young galaxies. Within the M…

astro-ph.CO20251 cited

Updated bounds on ultra-light dark matter from the tiniest galaxies

Simon May, Neal Dalal, Andrey Kravtsov

The particle mass of dark matter (DM) was previously constrained using kinematics of ultra-faint dwarf galaxies to . This constraint, which excl…

astro-ph.GA2025

Bursting at the seams: the star-forming main sequence and its scatter at z=3-9 using NIRCam photometry from JADES

C. Simmonds, S. Tacchella, W. McClymont +24

We present a comprehensive study of the star-forming main sequence (SFMS) and its scatter at redshifts , using NIRCam photometry from the JADES survey in the GOODS…

astro-ph.GA2025

Connecting JWST discovered N/O-enhanced galaxies to globular clusters: Evidence from chemical imprints

Xihan Ji, Vasily Belokurov, Roberto Maiolino +5

Recent JWST observations have revealed a growing population of galaxies at with elevated nitrogen-to-oxygen ratios. These "N/O-enhanced" galaxies (NOEGs) exhibit near- to sup…

astro-ph.GA202414 cited

Stochastic star formation and the abundance of UV-bright galaxies

Andrey Kravtsov, Vasily Belokurov

We use a well-motivated galaxy formation framework to predict stellar masses, star formation rates (SFR), and ultraviolet (UV) luminosities of galaxy populations at redshifts $z\in…