Deep Surveys and Cosmology

Details Deep Surveys and Cosmology Deep Surveys and Cosmology

1999-01-20

arxiv.org/abs/astro-ph/9901272v1

Astronomy and Astrophysics

Astrophysics

To appear in 'Highlights of the ISO Mission: Special Scientific Session of the IAU Gen. Assembly', ed. Lemke, D. et al. pub. K

Scientific paper

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.

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