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Deep Surveys and Cosmology

Published online by Cambridge University Press:  14 August 2015

S. J. Oliver ,
S. Sergeant ,
P. Goldschmidt ,
R.G. Mann ,
M. Rowan-Robinson ,
N. Eaton ,
A. Efsathiou ,
C. Gruppioni ,
T.J. Sumner  and
B. Mobasher
...Show all authors
S. J. Oliver
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
S. Sergeant
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
P. Goldschmidt
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
R.G. Mann
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
M. Rowan-Robinson
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
N. Eaton
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
A. Efsathiou
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
C. Gruppioni
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
T.J. Sumner
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
B. Mobasher
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
A. Verma
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
L. Danese
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
E. Egami
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
D. Elbaz
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
A. Franceschini
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
I. Gonzalez-Serrano
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
M. Kontizas
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
A. Lawrence
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
R. Mcmahon
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
H.U. Nørgaard-Nielsen
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine
I. Pérez-Fournon
Affiliation:
Astrophysics Group, Imperial College of Science Technology and Medicine

Extract

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Surveys with ISO (Kessler et al 1996), in particular with the CAM (Cesarsky et al 1996) and PHOT (Lemke et al 1996) instruments, will greatly extend our understanding of extra-galactic populations and their cosmological evolution. The main advantages that ISO surveys have over e.g IRAS are increased sensitivity/depth and wavelength coverage. Within the Guaranteed and Open Time programmes there are many field surveys which will efficiently map the limits in these parameters. In this talk I will briefly overview those surveys before concentrating in more detail on one survey in particular, the ISO survey of the Hubble Deep Field (HDF), to illustrate the kind of results that can be expected.

Type
III. Special Scientific Sessions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 1122 - 1124
Copyright
Copyright © Kluwer 1998

References

1. Bogun, S., et al., (1996), A&A, Vol. no. 315L, 71 Google Scholar
2. Cesarsky, C. J., et al., (1996), A&A, Vol. no. 315L, 32 Google Scholar
3. Connolly, A., Szalay, A.S., Dickinson, M., SubbaRao, M.U., Brunner, R.J. (1997) astro-ph/9706255Google Scholar
4. Elbaz, D., (1997), in Laureijs, R. & Levine, D., eds ‘Taking ISO to the Limits’ (ESA)Google Scholar
5. Franceschini, A., Mazzei, P., De Zotti, G., Giann, F., Danese, L., (1994), ApJ, Vol. no. 427, 140 Google Scholar
6. Goldschmidt, P., et al., (1997), MNRAS, Vol. no. 289, 465 CrossRefGoogle Scholar
7. Kawara, K., et al (1997), in Laureijs, R. & Levine, D., eds ‘Taking ISO to the Limits’ (ESA)Google Scholar
8. Kessler, M. F., et al., (1996), A&A, Vol. no. 315L, 27 Google Scholar
9. Lemke, D., et al., (1996), A&A, Vol. no. 315L, 64 Google Scholar
10. Lilly, S.J., Le Fevre, O., Hammer, F., Crampton, D., (1996), ApJ Vol. no. 460, LI CrossRefGoogle Scholar
11. Madau, , et al., (1996), MNRAS Vol. no. 283, 1388 CrossRefGoogle Scholar
12. Madau, P., Pozzetti, L., Dickinson, M., (1997), astro-ph/9708220Google Scholar
13. Mann, R.G., et al, (1997), MNRAS, Vol. no. 289, 482 Google Scholar
14. Nørgaard-Nielson, H.U., et al (1997), in Laureijs, R. & Levine, D., eds ‘Taking ISO to the Limits’ (ESA)Google Scholar
15. Oliver, S.J. et al, (1997a), MNRAS, Vol. no. 289, 471 Google Scholar
16. Oliver, S.J. et al. (1997b), in McLean, B. et al. eds, Proc. IAU Symp. 179, New Horizons …, Kluwer, Dordrecht Google Scholar
17. Pearson, C., Rowan-Robinson, M., (1996), MNRAS, Vol. no. 283, 174 CrossRefGoogle Scholar
18. Pei, Y.C., and Fall, S.M., (1995), ApJ Vol. no. 454, 69 CrossRefGoogle Scholar
19. Rowan-Robinson, M., et al., (1997), MNRAS, Vol. no. 289, 490 Google Scholar
20. Sergeant, S.B.G., et al, (1997), MNRAS, Vol. no. 289, 457 Google Scholar
21. Siebenmorgen, R.;, et al, (1996), A&A, Vol. no. 315L. 169 Google Scholar
22. Taniguichi, Y., et al (1997), in Laureijs, R. & Levine, D., eds ‘Taking ISO to the Limits’ (ESA)Google Scholar
23. Williams, R.E. et al., (1996), AJ, Vol. no. 112, 1335 Google Scholar