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Optical and Near-Infrared Imaging of the IRAS 1 Jy Sample of Ultraluminous Infrared Galaxies. I. The Atlas

D.-C. Kim et al 2002 ApJS 143 277-314   doi: 10.1086/343843  Help

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D.-C. Kim1, S. Veilleux2,3 and D. B. Sanders3,4
1 Current address: School of Earth and Environmental Sciences (BK21), Seoul National University, Seoul, Korea
2 Department of Astronomy, University of Maryland, College Park, MD 20742
3 Visiting Astronomer, W. M. Keck Observatory, jointly operated by the California Institute of Technology and the University of California
4 Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822; and Max-Planck-Institut für Extraterrestrische Physik, D-85740, Garching, Germany
E-mail: dckim@astro.snu.ac.kr, veilleux@astro.umd.edu and sanders@ifa.hawaii.edu

ABSTRACT. An imaging survey of the IRAS 1 Jy sample of 118 ultraluminous infrared galaxies was conducted at optical (R) and near-infrared (K') wavelengths using the University of Hawaii 2.2 m telescope. The methods of observation and data reduction are described. An R and K' atlas of the entire sample is presented along with some of the basic astrometric and photometric parameters derived from these images. A more detailed analysis of these data is presented in a companion paper.

Subject headings: galaxies: active; galaxies: interactions; galaxies: photometry; galaxies: Seyfert; galaxies: starburst; infrared: galaxies

An erratum for this article has been published in 2003 ApJS 147 221

Print publication: Issue 2 (2002 December)
Received 2002 June 6, accepted for publication 2002 July 31

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