activity
19952007
most citedThe GLARE Survey II. Faint z=6 Ly-alpha Line Emitters in the HUDF

72 citations · 73 across the 3 of their papers we have counts for

collaborators
Showing 2007Show all

7 papers · 1 filter

astro-ph2007109 cited

Effects of Dust Geometry in Lyman Alpha Galaxies at z = 4.4

Steven L. Finkelstein, James E. Rhoads, Sangeeta Malhotra +2

Equivalent widths (EWs) observed in high-redshift Lyman alpha galaxies could be stronger than the EW intrinsic to the stellar population if dust is present residing in clumps in th…

astro-ph20071 cited

Testing the Topology of Reionization

James E. Rhoads

The central overlap phase of cosmological hydrogen reionization is fundamentally a change in the topology of ionized regions. Before overlap, ionized bubbles grew in isolation. Dur…

astro-ph200720 cited

Infrared Emission from the Nearby Cool Core Cluster Abell 2597

Megan Donahue, Andres Jordan, Stefi A. Baum +9

We observed the brightest central galaxy (BCG) in the nearby (z=0.0821) cool core galaxy cluster Abell 2597 with the IRAC and MIPS instruments on board the Spitzer Space Telescope.…

astro-ph2007121 cited

A Luminosity Function of Lyman Alpha Emitting Galaxies at Redshift 4.5

Steve Dawson, James E. Rhoads, Sangeeta Malhotra +5

We present a catalog of 59 z=4.5 Lyman alpha emitting galaxies spectroscopically confirmed in a campaign of Keck/DEIMOS follow-up observations to candidates selected in the Large A…

astro-ph200711 cited

Chandra X-ray Sources in the LALA Cetus Field

J. X. Wang, Z. Y. Zheng, S. Malhotra +4

The 174 ks Chandra Advanced CCD Imaging Spectrometer exposure of the Large Area Lyman Alpha Survey (LALA) Cetus field is the second of the two deep Chandra images on LALA fields. I…

astro-ph200785 cited

Clustering of Lyman alpha emitters at z ~ 4.5

Katarina Kovač, Rachel S. Somerville, James E. Rhoads +2

We present the clustering properties of 151 Lyman alpha emitting galaxies at z ~ 4.5 selected from the Large Area Lyman Alpha (LALA) survey. Our catalog covers an area of 36' x 36'…