| Issue |
A&A
Volume 372, Number 3, June IV 2001
|
|
|---|---|---|
| Page(s) | L45 - L49 | |
| Section | Letters | |
| DOI | https://doi.org/10.1051/0004-6361:20010579 | |
| Published online | 15 June 2001 | |
The first ISO ERO: A dusty quasar at z = 1.5*
1
CEA Saclay, DSM/DAPNIA, Service d'Astrophysique, 91191 Gif-sur-Yvette, France
2
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
3
School of Physics, University of Sydney, NSW 2006, Australia
4
Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
Corresponding author: M. Pierre, This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
31
January
2001
Accepted:
23
April
2001
Abstract
We report the discovery of an extremely red object (ERO) in a medium-deep ISOCAM extragalactic survey. The object is also a radio source. Subsequent VLT NIR spectroscopy revealed a prominent Hα line giving a redshift of 1.5. We present the spectrum and photometric data points and discuss evidence that ISO J1324-2016 is a quasar harbouring a significant amount of very hot dust.
Key words: infrared: galaxies / quasars: general / galaxies: starburst / quasar: individual: ISO J1324-2016
Based on observations collected at the ISO Observatory, Canada-France-Hawaii Telescope, Australia Telescope Compact Array, UKIRT, ROSAT and the European Southern Observatory (prg: 58.E-0885, 61.B-0369, 265.B-5005).
© ESO, 2001
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