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25 April 2024
 
  » arxiv » astro-ph/0403458

 Article overview



GRAPES, Grism Spectroscopy of the Hubble Ultra Deep Field: Description and Data Reduction
N. Pirzkal ; C. Xu ; S. Malhotra ; J. E. Rhoads ; A. M. Koekemoer ; L. A. Moustakas ; J. R. Walsh ; R. A. Windhorst ; E. Daddi ; A. Cimatti ; H. C. Ferguson ; Jonathan P. Gardner ; C. Gronwall ; Z. Haiman ; M. K{ümmel ; N. Panagia ; A. Pasquali ; M. Stiavelli ; S. di Serego Alighieri ; Z. Tsvetanov ; J. Vernet ; H. Yan ;
Date 18 Mar 2004
Subject astro-ph
AbstractWe present deep unbiased spectroscopy of the Hubble Ultra Deep Field (UDF) carried out using the slitless grism spectroscopy mode of the Advance Camera for Surveys on the Hubble Space Telescope (HST). The GRIsm ACS Program for Extragalactic Science (GRAPES) achieves continuum detection as faint as $z_{AB}=27.2$ using 40 orbits ($9.2 imes 10^4$ seconds) on HST. The data were taken at four orientation angles to correct for the overlap of spectra. GRAPES data provide a unique, uninterrupted, low resolution (R=100) spectral coverage for $5500AA < lambda < 10500AA$, and allow us to detect high redshift galaxies at $4 < z < 7$ whether they have $lya$ lines or just show the Lyman Break, as well as find low luminosity AGNs in an unbiased fashion. This paper describes in detail the observations and the data reduction, and examines the quality of the extracted spectra. Subsequent papers will deal with the analysis of the data. The extracted and calibrated GRAPES spectra will be available from MAST at STScI.
Source arXiv, astro-ph/0403458
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