activity
19992017
most citedEvolution of Interstellar Medium, Star Formation, and Accretion at High Redshift

348 citations · 1.9k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2017★ 348 cited

Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift

N. Scoville, N. Lee, P. Vanden Bout +20

ALMA observations of the long wavelength dust continuum are used to estimate the interstellar medium (ISM) masses in a sample of 708 galaxies at z = 0.3 to 4.5 in the COSMOS field.…

astro-ph.IM2016★ 12 cited

The Far-Infrared Surveyor Mission Study: Paper I, the Genesis

M. Meixner, A. Cooray, R. Carter +27

This paper describes the beginning of the Far-Infrared Surveyor mission study for NASA's Astrophysics Decadal 2020. We describe the scope of the study, and the open process approac…

astro-ph.GA2010★ 179 cited

Mid-Infrared Spectral Diagnostics of Luminous Infrared Galaxies

A. O. Petric, L. Armus, J. Howell +22

We present a statistical analysis of the mid-infrared (MIR) spectra of 248 luminous infrared (IR) galaxies (LIRGs) which comprise the Great Observatories All-sky LIRG Survey (GOALS…

astro-ph.GA2010★ 315 cited

Black hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231

P. P. Van der Werf, K. G. Isaak, R. Meijerink +34

We present a full high resolution SPIRE FTS spectrum of the nearby ultraluminous infrared galaxy Mrk231. In total 25 lines are detected, including CO J=5-4 through J=13-12, 7 rotat…

astro-ph.GA2009★ 63 cited

High-ionization Fe K emission from luminous infrared galaxies

K. Iwasawa, D. B. Sanders, A. S. Evans +3

The Chandra component of the Great Observatories All-Sky LIRG Survey (GOALS) presently contains 44 luminous and ultraluminous infrared galaxies with log (Lir/Lsun) = 11.73-12.57. O…

astro-ph2008★ 22 cited

The Origin of the 24-micron Excess in Red Galaxies

Kate Brand, John Moustakas, Lee Armus +11

Observations with the Spitzer Space Telescope have revealed a population of red-sequence galaxies with a significant excess in their 24-micron emission compared to what is expected…