activity
19992013
most citedObservations of Ultraluminous Infrared Galaxies with the Infrared Spectrograph on the Spitzer Space Telescope: Early Results on Mrk 1014, Mrk 463, and UGC 5101

132 citations · 178 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO2013★ 27 cited

The 2nd Generation z(Redshift) and Early Universe Spectrometer Part I: First-light observation of a highly lensed local-ULIRG analog at high-z

Carl Ferkinhoff, Drew Brisbin, Stephen Parshley +20

We report first science results from our new spectrometer, the 2nd generation z(Redshift) and Early Universe Spectrometer (ZEUS-2), recently commissioned on the Atacama Pathfinder…

astro-ph2005★ 18 cited

Radio Observations of the Hubble Deep Field South region: I. Survey Description and Initial Results

Ray P. Norris, Minh T. Huynh, Carole A. Jackson +8

This paper is the first of a series describing the results of the Australia Telescope Hubble Deep Field South (ATHDFS) radio survey. The survey was conducted at four wavelengths -…

astro-ph2004★ 132 cited

Observations of Ultraluminous Infrared Galaxies with the Infrared Spectrograph on the Spitzer Space Telescope: Early Results on Mrk 1014, Mrk 463, and UGC 5101

L. Armus, V. Charmandaris, H. W. W. Spoon +2

We present spectra taken with the Infrared Spectrograph on Spitzer covering the 5-38micron region of three Ultraluminous Infrared Galaxies (ULIRGs): Mrk 1014 (z=0.163), and Mrk 463…

astro-ph2004

Spitzer/IRS Observations of the Redshift 3.91 quasar APM 08279+5255

B. T. Soifer, V. Charmandaris, B. R. Brandl +14

The Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope (SST) has been used to obtain low and moderate resolution spectra of the dust and gas-rich quasar APM08279+5255…

astro-ph1999★ 1 cited

Radio Observations of the Hubble Deep Field South - a New Class of Radio-Luminous Galaxies?

R. P. Norris, A. Hopkins, R. J. Sault +7

We present the first results from a series of radio observations of the Hubble Deep Field South and its flanking fields. Here we consider only those sources greater than 100 microJ…