Copy the page URI to the clipboard
Morel, T.; Efstathiou, A.; Serjeant, S.; Márquez, I.; Masegosa, J. and Héraudeau, P. [et al.]
(2001).
DOI: https://doi.org/10.1046/j.1365-8711.2001.04803.x
URL: http://arxiv.org/abs/astro-ph/0107148
Abstract
We report the discovery of the first hyperluminous infrared galaxy (HyLIG) in the course of the European Large Area ISO Survey (ELAIS). This object has been detected by ISO at 6.7, 15 and 90mum, and is found to be a broad-line, radio-quiet quasar at a redshift [formmu4]z=1.099. From a detailed multicomponent model fit of the spectral energy distribution, we derive a total IR luminosity LIR [formmu5](1-1000mum)~1.0×1013h65-2Lsolar [formmu6](q0=0.5), and discuss the possible existence of a starburst contributing to the far-IR output. Observations to date present no evidence for lens magnification. This galaxy is one of the very few HyLIGs with a X-ray detection. On the basis of its soft X-ray properties, we suggest that this broad-line object may be the face-on analogue of narrow-line, Seyfert-like HyLIGs.
Viewing alternatives
Metrics
Public Attention
Altmetrics from AltmetricNumber of Citations
Citations from DimensionsItem Actions
Export
About
- Item ORO ID
- 5810
- Item Type
- Journal Item
- ISSN
- 1365-2966
- Extra Information
- Some of the symbols may not have transferred correctly into this bibliographic record and/or abstract.
- Keywords
- Quasars; ELAISP90;_J164010+410502 ([CCS88]; 163831.4+411107); surveys; galaxies; starburst; infrared
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
- ?? space ??
- Depositing User
- Users 13 not found.