activity
19962024
most citedStarburst99: Synthesis Models for Galaxies with Active Star Formation

4k citations · 12.4k across the 59 of their papers we have counts for

collaborators

60 papers

astro-ph.GA2024

UVCANDELS: Catalogs of photometric redshifts and galaxy physical properties

Vihang Mehta, Marc Rafelski, Ben Sunnquist +76

The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep HST F275W and F435W imaging over four CANDELS…

astro-ph.GA2023★ 15 cited

The UV luminosity function at 0.6 < z < 1 from UVCANDELS

Lei Sun, Xin Wang, Harry I. Teplitz +75

UVCANDELS is a HST Cycle-26 Treasury Program awarded 164 orbits of primary ultraviolet (UV) F275W imaging and coordinated parallel optical F435W imaging in four CANDELS fields: GOO…

astro-ph.GA2019★ 18 cited

Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field

Tommy Wiklind, Henry C. Ferguson, Yicheng Guo +12

We present an ALMA survey of dust continuum emission in a sample of 70 galaxies in the redshift range z=2-5 selected from the CANDELS GOODS-S field. Multi-Epoch Abundance Matching…

astro-ph.GA2017★ 114 cited

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…

astro-ph.GA2017★ 49 cited

UVUDF: UV Luminosity Functions at the cosmic high-noon

Vihang Mehta, Claudia Scarlata, Marc Rafelski +14

We present the rest-1500Å UV luminosity functions (LF) for star-forming galaxies during the cosmic \textit{high noon} -- the peak of cosmic star formation rate at . We use…

astro-ph.GA2016★ 77 cited

Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5<z<3

Peter Kurczynski, Eric Gawiser, Viviana Acquaviva +16

We present estimates of intrinsic scatter in the Star Formation Rate (SFR) - Stellar Mass (M*) correlation in the redshift range 0.5 < z < 3.0 and in the mass range 10^7 < M* < 10^…