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The STIS Parallel Survey: Introduction and First Results
Author(s) -
Jonathan P. Gardner,
Robert Hill,
Stefi A. Baum,
Nicholas R. Collins,
Henry C. Ferguson,
R. A. E. Fosbury,
Ronald L. Gilliland,
Richard F. Green,
T. R. Gull,
Sara R. Heap,
Don J. Lindler,
E. M. Malumuth,
A. Micol,
N. Pirzkal,
Jennifer Sandoval,
Eline Tolstoy,
J. R. Walsh,
B. E. Woodgate
Publication year - 1998
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/311105
Subject(s) - space telescope imaging spectrograph , galaxy , redshift , physics , astrophysics , spectrograph , hubble ultra deep field , hubble deep field south , hubble space telescope , astronomy , grism , spectroscopy , star formation , observational cosmology , hubble deep field , spectral line
The installation of the Space Telescope Imaging Spectrograph (STIS) on theHubble Space Telescope (HST) allows for the first time two-dimensional opticaland ultraviolet slitless spectroscopy of faint objects from space. The STISParallel Survey (SPS) routinely obtains broad band images and slitless spectraof random fields in parallel with HST observations using other instruments. TheSPS is designed to study a wide variety of astrophysical phenomena, includingthe rate of star formation in galaxies at intermediate to high redshift throughthe detection of emission-line galaxies. We present the first results of theSPS, which demonstrate the capability of STIS slitless spectroscopy to detectand identify high-redshift galaxies.Comment: 11 pages, Latex, 3 enclosed Postscript figures, aaspp4.sty, accepted for publication in the Astrophysical Journal Letters HST Second Servicing Mission special issu

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