activity
20042009
most citedUV Star Formation Rates in the Local Universe

1.7k citations · 5.2k across the 31 of their papers we have counts for

collaborators

60 papers

astro-ph.CO200913 cited

Probing the Intermediate-Age Globular Clusters in NGC 5128 from Ultraviolet Observations

Soo-Chang Rey, Sangmo T. Sohn, Michael A. Beasley +23

We explore the age distribution of the globular cluster (GC) system of the nearby elliptical galaxy NGC 5128 using ultraviolet (UV) photometry from Galaxy Evolution Explorer (GALEX…

astro-ph.GA200911 cited

Studying Large and Small Scale Environments of Ultraviolet Luminous Galaxies

Antara R. Basu-Zych, David Schiminovich, Sebastien Heinis +23

Studying the environments of 0.4<z<1.2 UV-selected galaxies, as examples of extreme star-forming galaxies (with star formation rates in the range of 3-30 M_sol/yr), we explore the…

astro-ph.CO200957 cited

GALEX-SDSS Catalogs for Statistical Studies

T. Budavari, S. Heinis, A. S. Szalay +23

We present a detailed study of the Galaxy Evolution Explorer's photometric catalogs with special focus on the statistical properties of the All-sky and Medium Imaging Surveys. We i…

astro-ph2008114 cited

Probing Shock Breakout with Serendipitous GALEX Detections of Two SNLS Type II-P Supernovae

Suvi Gezari, Luc Dessart, Stephane Basa +13

We report the serendipitous detection by GALEX of fast (<1 day) rising (>1 mag) UV emission from two Type II plateau (II-P) supernovae (SNe) at z=0.185 and 0.324 discovered by the…

astro-ph200894 cited

Lyman alpha emitting galaxies at 0.2 < z < 0.35 from GALEX spectroscopy

Jean-Michel Deharveng, Todd Small, Tom A. Barlow +19

The GALEX (Galaxy Evolution Explorer) spectroscopic survey mode, with a resolution of about 8 A in the FUV (1350 - 1750 A) and about 20 A in the NUV (1950 - 2750 A) is used for a s…

astro-ph200782 cited

Ultraviolet through Infrared Spectral Energy Distributions from 1000 SDSS Galaxies: Dust Attenuation

Benjamin D. Johnson, David Schiminovich, Mark Seibert +19

The meaningful comparison of models of galaxy evolution to observations is critically dependent on the accurate treatment of dust attenuation. To investigate dust absorption and em…