activity
20042024
most citedThe UV-optical Galaxy Color-Magnitude Diagram I: Basic Properties

436 citations · 2.2k across the 15 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2024★ 10 cited

Distribution of merging and post-merging galaxies in nearby galaxy clusters

Duho Kim, Yun-Kyeong Sheen, Yara L. Jaffé +10

We study the incidence and spatial distribution of galaxies that are currently undergoing gravitational merging (M) or that have signs of a post merger (PM) in six galaxy clusters…

astro-ph.CO2010★ 188 cited

HST WFC3/IR Observations of Active Galactic Nucleus Host Galaxies at z~2: Supermassive Black Holes Grow in Disk Galaxies

Kevin Schawinski, Ezequiel Treister, C. Megan Urry +3

We present the rest-frame optical morphologies of active galactic nucleus (AGN) host galaxies at 1.5<z<3, using near-infrared imaging from the Hubble Space Telescope Wide Field Cam…

astro-ph.CO2010★ 27 cited

The UV-Optical Color Dependence of Galaxy Clustering in the Local Universe

Yeong-Shang Loh, R. Michael Rich, Sébastien Heinis +22

We measure the UV-optical color dependence of galaxy clustering in the local universe. Using the clean separation of the red and blue sequences made possible by the NUV - r color-m…

astro-ph.CO2009★ 24 cited

Spatial Clustering from GALEX-SDSS samples: Star Formation History and large-scale clustering

Sebastien Heinis, Tamas Budavari, Alex S. Szalay +19

We measure the projected spatial correlation function w_p(r_p) from a large sample combining GALEX ultraviolet imaging with the SDSS spectroscopic sample. We study the dependence o…

astro-ph2008★ 94 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-ph2007★ 51 cited

Ultraviolet, Optical, and Infrared Constraints on Models of Stellar Populations and Dust Attenuation

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

The color of galaxies is a fundamental property, easily measured, that constrains models of galaxies and their evolution. Dust attenuation and star formation history (SFH) are the…