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Starburst Galaxies: Near and Far pp 297–302Cite as

Identification of ISOPHOT Deep Field Sources

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Part of the book series: Springer Proceedings in Physics ((SPPHY,volume 88))

Abstract

We have completed an analysis of the deepest far-infrared (90 (μm,175 μm) survey made using the ISOPHOT photometer aboard the Infrared Space Observatory (ISO). The cumulative number counts for two 44′ x 44′ regions in the Lockman Hole appear to be ~ 10 times higher than expected from a no-evolution model. Optical counterparts for the brightest 175 μm sources, ( S 175 > 150 mJy), have recently been identified using I-band and K-band imaging plus VLA-B 20cm continuum maps. Keck spectroscopy of a subsample of these sources shows that they are dusty emission line galaxies at redshifts z < 1.5, with infrared luminosities1 in the range L ir ~ 1010 – 1013 L ⊙. These ISOPHOT sources plausibly represent a link between the low-z luminous infrared galaxies (LIGs) detected by IRAS and the more distant submillimeter sources that have recently been detected in deep 850 μm surveys with SCUBA.

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Author information

Authors and Affiliations

  1. Institute for Astronomy, Univ. of Hawaii, 2680 Woodlawn Dr., Honolulu, HI, 96822, USA

    David B. Sanders & Lennox L. Cowie

  2. Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, 85741, Garching, Germany

    David B. Sanders

  3. Department of Astronomy, University of Maryland, College Park, MD, 20742, USA

    Sylvain Veilleux

  4. Department of Astronomy, University of Massachusetts, Amherst, MA, 01003, USA

    Min Yun

  5. Institute of Astronomy, U. Tokyo, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan

    Kimiaki Kawara & Shinki Oyabu

  6. Astronomical Institute, Tohoku University, Aoba, Sendai, 980-8578, Japan

    Yoshiaki Taniguchi & Takashi Murayama

  7. Gunma Astronomical Observatory, 6860-86 Nakayama, Takayama, Agatsuma, Gunma, 371-0702, Japan

    Haruyuki Okuda

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  1. David B. Sanders
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  2. Sylvain Veilleux
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  3. Min Yun
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  4. Lennox L. Cowie
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  5. Kimiaki Kawara
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  6. Yoshiaki Taniguchi
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  7. Shinki Oyabu
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  8. Takashi Murayama
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  9. Haruyuki Okuda
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Editor information

Editors and Affiliations

  1. Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, 85741, Garching, Germany

    Linda Tacconi  & Dieter Lutz  & 

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© 2001 Springer-Verlag Berlin Heidelberg

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Sanders, D.B. et al. (2001). Identification of ISOPHOT Deep Field Sources. In: Tacconi, L., Lutz, D. (eds) Starburst Galaxies: Near and Far. Springer Proceedings in Physics, vol 88. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-56538-0_42

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  • DOI: https://doi.org/10.1007/978-3-642-56538-0_42

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-62562-6

  • Online ISBN: 978-3-642-56538-0

  • eBook Packages: Springer Book Archive

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