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Ground-Based Photometric Calibration of the Space Telescope CCD Camera

Published online by Cambridge University Press:  14 August 2015

D.A. Hunter ,
H.C. Harris ,
W.A. Baum ,
J.H. Jones  and
T.J. Kreidl
D.A. Hunter
Affiliation:
Lowell Observatory, 1400 West Mars Hill Rd., Flagstaff, AZU.S.A.
H.C. Harris
Affiliation:
U.S. Naval Observatory, PO Box 1149, Flagstaff, AZU.S.A.
W.A. Baum
Affiliation:
Lowell Observatory, 1400 West Mars Hill Rd., Flagstaff, AZU.S.A.
J.H. Jones
Affiliation:
Lowell Observatory, 1400 West Mars Hill Rd., Flagstaff, AZU.S.A.
T.J. Kreidl
Affiliation:
Lowell Observatory, 1400 West Mars Hill Rd., Flagstaff, AZU.S.A.

Extract

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The Wide-Field and Planetary Camera (WF/PC) is a CCD imaging instrument which is part of the Hubble Space Telescope. Ground-based observations have been made with a CCD system similar to those of the WF/PC in order to establish the standard star sequence to be used for in-flight photometric calibration. Because the WF/PC passbands differ from those in previous photometric use, the filters and CCDs will define a new photometric system. We outline here the procedures used to establish the calibration fields to be used in flight (see Harris et al. 1988 for additional details).

Type
Joint Commission Meeting
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 631 - 634
Copyright
Copyright © Kluwer 1989

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