Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasp..106..646k&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 106, no. 700, p. 646-669
Astronomy and Astrophysics
Astronomy
27
Absorption Spectra, Position (Location), Quasars, Satellite-Borne Photography, Astrometry, Astronomical Photometry, Astronomical Spectroscopy, Charge Coupled Devices, Classifications, Galaxies, Hubble Space Telescope, Red Shift, Stars, Stellar Magnitude
Scientific paper
We present an analysis of CCD images of more than 100 quasars; many of the objects have been or will be observed in the Hubble Space Telescope (HST) Key Project Quasar Absorption-Line Survey. The data set consists of B, g, and i photometry of 117 quasars and deeper g (limiting magnitude of approximately equal 22) images of 101 quasar fields. Positions accurate to approximately equal 1 sec, measured with the Space Telescope Science Institute's Astrometric Support Program, are listed for all of the quasars in this study. Positions, magnitudes, and classifications of stars and galaxies located within approximately equal 100 sec of the quasars are given for all of the deep g data. The positions of the stars and galaxies relative to the quasar are accurate to approximately equal 0.5 sec. The results presented here can be used to prepare spectroscopic programs designed to obtain redshifts of galaxies in the fields of these quasars.
Bahcall John N.
Jannuzi Buell Tomasson
Kirhakos Sofia
Maoz Dan
Sargent Wallace L. W.
No associations
LandOfFree
The HST Quasar Absorption-Line Key Project. 8: CCD imaging of Hubble Space Telescope quasar fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The HST Quasar Absorption-Line Key Project. 8: CCD imaging of Hubble Space Telescope quasar fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The HST Quasar Absorption-Line Key Project. 8: CCD imaging of Hubble Space Telescope quasar fields will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1507207