The European large area ISO survey -: III.: 90-μm extragalactic source counts

被引:63
作者
Efstathiou, A
Oliver, S
Rowan-Robinson, M
Surace, C
Sumner, T
Héraudeau, P
Linden-Vornle, MJD
Rigopoulou, D
Serjeant, S
Mann, RG
Cesarsky, CJ
Danese, L
Franceschini, A
Genzel, R
Lawrence, A
Lemke, D
McMahon, RG
Miley, G
Puget, JL
Rocca-Volmerange, B
机构
[1] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England
[2] Univ Sussex, Ctr Astron, Brighton BN1 9QH, E Sussex, England
[3] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[4] Danish Space Res Inst, DK-2100 Copenhagen O, Denmark
[5] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[6] CEA Saclay, F-91191 Gif Sur Yvette, France
[7] SISSA, Int Sch Adv Studies, I-34014 Trieste, Italy
[8] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
[9] Univ Edinburgh, Royal Observ, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
[10] Univ Cambridge, Inst Astron, The Observ, Cambridge CB3 0HA, England
[11] Leiden Observ, NL-2300 RA Leiden, Netherlands
[12] Univ Paris 11, Inst Astrophys Spatiale, F-91405 Orsay, France
[13] Inst Astrophys, F-75014 Paris, France
关键词
surveys; galaxies : evolution; galaxies : formation; galaxies : Seyfert; galaxies : starburst; infrared : galaxies;
D O I
10.1046/j.1365-8711.2000.03914.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results and source counts at 90 mum extracted from the preliminary analysis of the European Large Area ISO Survey (ELAIS). The survey covered about 12 deg(2) of the sky in four main areas and was carried out with the ISOPHOT instrument onboard the Infrared Space Observatory (ISO). The survey is at least an order of magnitude deeper than the IRAS 100-mum survey and is expected to provide constraints on the formation and evolution of galaxies. The majority of the detected sources are associated with galaxies on optical images. In some cases the optical associations are interacting pairs or small groups of galaxies, suggesting that the sample may include a significant fraction of luminous infrared galaxies. The source counts extracted from a reliable subset of the detected sources are in agreement with strongly evolving models of the starburst galaxy population.
引用
收藏
页码:1169 / 1177
页数:9
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