The European Large Area ISO Survey -: I.: Goals, definition and observations

被引:185
|
作者
Oliver, S
Rowan-Robinson, M
Alexander, DM
Almaini, O
Balcells, M
Baker, AC
Barcons, X
Barden, M
Bellas-Velidis, I
Cabrera-Guerra, F
Carballo, R
Cesarsky, CJ
Ciliegi, P
Clements, DL
Crockett, H
Danese, L
Dapergolas, A
Drolias, B
Eaton, N
Efstathiou, A
Egami, E
Elbaz, D
Fadda, D
Fox, M
Franceschini, A
Genzel, R
Goldschmidt, P
Graham, M
Gonzalez-Serrano, JI
Gonzalez-Solares, EA
Granato, GL
Gruppioni, C
Herbstmeier, U
Héraudeau, P
Joshi, M
Kontizas, E
Kontizas, M
Kotilainen, JK
Kunze, D
La Franca, F
Lari, C
Lawrence, A
Lemke, D
Linden-Vornle, MJD
Mann, RG
Márquez, I
Masegosa, J
Mattila, K
McMahon, RG
Miley, G
机构
[1] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2BZ, England
[2] SISSA, Int Sch Adv Studies, I-34014 Trieste, Italy
[3] Univ Edinburgh, Royal Observ, Astron Inst, Edinburgh EH9 3JH, Midlothian, Scotland
[4] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, SC De Tenerife, Spain
[5] Cardiff Univ, Dept Phys & Astron, Cardiff CF24 3YB, S Glam, Wales
[6] Univ Cantabria, CSIC, Inst Fus Cantabria, E-39005 Santander, Spain
[7] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[8] Natl Observ Athens, Inst Astron, GR-11810 Athens, Greece
[9] Univ Cantabria, Dept Fus Moderna, E-39005 Santander, Spain
[10] CEA Saclay, F-91191 Gif Sur Yvette, France
[11] Osservatorio Astron Bologna, I-40127 Bologna, Italy
[12] CALTECH, Infrared Astron Grp, Downs Lab Phys 320 47, Pasadena, CA 91125 USA
[13] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
[14] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[15] Univ Athens, Dept Phys, Sect Astrophys Astron & Mech, GR-15783 Zografos, Greece
[16] Univ Turku, Tuorla Observ, FIN-21500 Piikkio, Finland
[17] Univ Roma TRE, Dipartimento Fis, I-00146 Rome, Italy
[18] Inst Radio Astron, Bologna, Italy
[19] Astron Observ, Niels Bohr Inst Astron Phys & Geophys, DK-2100 Copenhagen O, Denmark
[20] Danish Space Res Inst, DK-2100 Copenhagen O, Denmark
[21] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[22] Observ, FIN-00014 Helsinki, Finland
[23] Univ Cambridge Inst Astron, Inst Astron, Cambridge CB3 0HA, England
[24] Inst Astrophys Paris, F-75014 Paris, France
[25] Univ Paris 11, Inst Astrophys Spatiale, F-91405 Orsay, France
关键词
surveys; galaxies : active; galaxies : evolution; galaxies : starburst; infrared : galaxies; infrared : stars;
D O I
10.1046/j.1365-8711.2000.03550.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe the European Large Area ISO Survey (ELAIS). ELAIS was the largest single Open Time project conducted by ISO, mapping an area of 12 deg(2) at 15 mu m with ISOCAM and at 90 mu m with ISOPHOT. Secondary surveys in other ISO bands were undertaken by the ELAIS team within the fields of the primary survey, with 6 deg(2) being covered at 6.7 mu m and 1 deg(2) at 175 mu m. This paper discusses the goals of the project and the techniques employed in its construction, as well as presenting details of the observations carried out, the data from which are now in the public domain. We outline the ELAIS 'preliminary analysis' which led to the detection of over 1000 sources from the 15 and 90-mu m surveys (the majority selected at 15 mu m with a flux limit of similar to 3 mJy), to be fed into a ground-based follow-up campaign, as well as a programme of photometric observations of detected sources using both ISOCAM and ISOPHOT. We detail how the ELAIS survey complements other ISO surveys in terms of depth and areal coverage, and show that the extensive multi-wavelength coverage of the ELAIS fields resulting from our concerted and on-going follow-up programme has made these regions amongst the best studied areas of their size in the entire sky, and, therefore, natural targets for future surveys. This paper accompanies the release of extremely reliable subsets of the 'preliminary analysis' products. Subsequent papers in this series will give further details of our data reduction techniques, reliability and completeness estimates and present the 15- and 90-mu m number counts from the 'preliminary analysis', while a further series of papers will discuss in detail the results from the ELAIS 'final analysis', as well as from the follow-up programme.
引用
收藏
页码:749 / 767
页数:19
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