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Molecular Gas in 3C 293: The First Detection of CO Emission and Absorption in an F-R II Radio Galaxy
A. S. Evans, D. B. Sanders, J. A. Surace +1
The first detection of CO emission in a Fanaroff-Riley Class II (i.e., edge-brightened radio morphology) radio galaxy is presented. Multi- wavelength (0.36-2.17 micron) imaging of…
Dusty star forming galaxies at high redshift
A. J. Barger, L. L. Cowie, D. B. Sanders +5
The global star formation rate in high redshift galaxies, based on optical surveys, shows a strong peak at a redshift of z=1.5, which implies that we have already seen most of the…
The IRAS 1-Jy Survey of Ultraluminous Infrared Galaxies: II. Optical Spectroscopy
D. -C. Kim, S. Veilleux, D. B. Sanders
This is the second paper in a series discussing the properties of ultraluminous infrared galaxies (ULIGs: L_ir > 10^{12} L_sun; Ho = 75 km s^{-1} Mpc^{-1} and qo = 0.0) from the 1-…
The IRAS 1-Jy Survey of Ultraluminous Infrared Galaxies: I. The sample and Luminosity Function
D. -C. Kim, D. B. Sanders
A complete flux-limited sample of 118 ultraluminous infrared galaxies (ULIGs) has been identified from the IRAS Faint Source Catalog (FSC). The selection criteria were a 60 micron…
NIR Spectroscopy and a Search for CO Emission in Three Extremely Luminous IRAS Sources; IR 09105+4108, IR 15307+3252, and PG 1634+706
A. S. Evans, D. B. Sanders, R. M. Cutri +5
Rest-frame 0.48-1.1 micron emission line strengths and molecular gas mass (H_2) upper limits for 3 luminous infrared sources - the hyperluminous infrared galaxies IR F09105+4108 (z…
Near-Infrared Spectroscopy of the High Redshift Quasar S4 0636+68 at z=3.2
Takashi Murayama, Yoshiaki Taniguchi, Aaron S. Evans +4
We present near-infrared (observed frame) spectra of the high-redshift quasar S4 0636+68 at z=3.2 which was previously thought to be one of a group of ``strong'' Fe II emitters [i.…