Reference : Mid-FIR Properties of ELAIS Sources
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/32092
Mid-FIR Properties of ELAIS Sources
English
Marquez, I. [ > > ]
Masegosa, J. [Instituto de Astrofísica de Andalucía, Apdo 3004, 18080 Granada (Spain)]
Morel, Thierry [Astrophysics Group, Imperial College of Science, Technology and Medicine, Blackett Laboratory, Prince Consort Road, London SW7 2BZ > > > >]
Efstathiou, A. [Astrophysics Group, Imperial College of Science, Technology and Medicine, Blackett Laboratory, Prince Consort Road, London, SW7 2BZ, UK]
Verma, A. [Astrophysics Group, Imperial College of Science, Technology and Medicine, Blackett Laboratory, Prince Consort Road, London, SW7 2BZ, UK]
Vaisanen, P. [Observatory, P.O. Box 14, Tahtitorninmaki, FIN-00014, University of Helsinki, Finland]
Alexander, D. [SISSA, International School for Advanced Studies, Via Beirut 2-4, 34014 Trieste, Italy]
Heraudeau, P. [ > > ]
Surace, C. [Astrophysics Group, Imperial College of Science, Technology and Medicine, Blackett Laboratory, Prince Consort Road, London, SW7 2BZ, UK]
Perez-Fournon, I. [ > > ]
Cabrera-Guerra, F. [Instituto de Astrofísica de Canarias, Vía Láctea s/n, 38200 La Laguna, Tenerife, Canary Islands, Spain]
Gonzalez-Serrano, J. I. [ > > ]
Gonzalez-Solares, E. A. [ > > ]
Serjeant, S. [Astrophysics Group, Imperial College of Science, Technology and Medicine, Blackett Laboratory, Prince Consort Road, London, SW7 2BZ, UK]
Oliver, S. J. [Astronomy Center, University of Sussex, Falmer, Brighton, BN1 9QJ, UK]
Rowan-Robinson, M. [Astrophysics Group, Imperial College of Science, Technology and Medicine, Blackett Laboratory, Prince Consort Road, London, SW7 2BZ, UK]
1-Jul-2001
The Promise of the Herschel Space Observatory
147
No
International
[en] GALAXIES: INFRARED: COLORS ; GALAXIES: SURVEYS ; GALAXIES: STARBURSTS ; ACTIVE
[en] We present the properties of all the galaxies detected by ISO at 7, 15 and 90 microns in ELAIS northern fields. The spectral energy distribution (SED) of those 20 galaxies with IRAS detections can generally be well fitted by a predominant cirrus component plus a modest starburst contribution. Follow-up spectroscopy has shown that all the objects are emission-line galaxies but without a very intense star formation event. Most of the galaxies analyzed by means of optical R band photometry result to host an important exponential disk component, in good agreement with the SED IR modelling. We note that galaxies with morphological signs of perturbations seem to show slightly higher f[SUB]15[/SUB]/f[SUB]6.7[/SUB] ratios, indicating that star formation could be more important in them. One of the objects is a broad-line, radio-quiet quasar at z=1.099; its spectral energy distribution indicates that it is a hyperluminous infrared galaxy (HLIG), the first HLIG detected in the ELAIS areas.
http://hdl.handle.net/2268/32092
http://adsabs.harvard.edu/abs/2001ESASP.460..147M
460

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