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Astrophysics

Title: The VLT observations of the HDF-S NICMOS field: photometric catalog and high redshift galaxy candidates

Authors: A. Fontana (1), S. D'Odorico (2), R. Fosbury (3), E. Giallongo (1), R. Hook (3), F. Poli (1), A. Renzini (2), P. Rosati (2), R. Viezzer (2) ((1) Osservatorio Astronomico di Roma (2) ESO (3) ST-ECF)
Abstract: We present the deep UBVRI observations of the HDF-S NICMOS field obtained as part of the Science Verification of the VLT Unit 1 telescope. The images have been used to construct object catalogs and to obtain photometric redshifts. The effective field of view is $\simeq 70\times70$ arcsec$^2$, and the formal $5\sigma$ limiting magnitudes (in a 2 FWHM aperture) are 26.3, 27.8, 27.5, 26.9, 25.2 in the $U$, $B$, $V$, $R$ and $I$ bands, respectively. Thanks to the sub-arcsecond image quality, relatively long exposure time, and large collecting area of the VLT, this is the deepest set of multicolor images ever obtained from a ground-based telescope. Galaxy counts have been derived independently in each band, and show no significant departures from previous data from wider areas. A multicolor photometric catalog of all the galaxies selected in the $R$ band has also been obtained and used to derive photometric redshifts for all galaxies with $R \leq 26.5 $, using also the J,H and K magnitudes from the NICMOS deep observations. A significant fraction (\simeq 28%)of the galaxies is placed at $z\geq 2$. Among them, six robust candidates are found at $z \geq 2.5$ .
Comments: Accepted on A&A Letters, Special VLT Letter section in March 1999
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/9901359v1

Submission history

From: Adriano Fontana [view email]
[v1] Tue, 26 Jan 1999 16:59:04 GMT (83kb)