activity
19992025
most citedLy Alpha-Emitting Galaxies at z=3.1: L* Progenitors Experiencing Rapid Star Formation

321 citations · 590 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2025★ 3 cited

Mid-infrared extinction toward the Galactic center

Sebastiano D. von Fellenberg, Joseph M. Michail, S. P. Willner +10

We determine the mid-infrared (MIR, 5~μm--22~μm) extinction towards the Galactic center using MIRI/MRS integral field unit (IFU) observations of the central re…

astro-ph.SR2015

SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment

J. D. Adams, T. L. Herter, J. L. Hora +22

We present mid-IR (19 - 37 microns) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6 - 8.0 microns), IRTF/MIRLIN (11.3 and…

astro-ph.HE2015★ 160 cited

AEGIS-X: Deep Chandra imaging of the Central Groth Strip

K. Nandra, E. S. Laird, J. A. Aird +22

We present the results of deep \chandra\ imaging of the central region of the Extended Groth Strip, the AEGIS-X Deep (AEGIS-XD) survey. When combined with previous \chandra\ observ…

astro-ph2007★ 321 cited

Ly Alpha-Emitting Galaxies at z=3.1: L* Progenitors Experiencing Rapid Star Formation

Eric Gawiser, Harold Francke, Kamson Lai +18

We studied the clustering properties and multiwavelength spectral energy distributions of a complete sample of 162 Ly Alpha-Emitting (LAE) galaxies at z=3.1 discovered in deep narr…

astro-ph2006★ 82 cited

The Stellar Population of Lyman-alpha Emitting Galaxies at z ~ 5.7

Kamson Lai, Jia-Sheng Huang, Giovanni Fazio +3

We present a study of three Lyman-alpha emitting galaxies (LAEs), selected via a narrow-band survey in the GOODS northern field, and spectroscopically confirmed to have redshifts o…

astro-ph2005★ 24 cited

Why Optically--Faint AGN Are Faint: The Spitzer Perspective

J. R. Rigby, G. H. Rieke, P. G. Perez-Gonzalez +5

Optically--faint X-ray sources (those with f_X/f_R > 10) constitute about 20% of X-ray sources in deep surveys, and are potentially highly obscured and/or at high redshift. Their f…