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Astrometry of Poss-II Plates Using Tycho

Published online by Cambridge University Press:  14 August 2015

B. Bucciarelli
Affiliation:
1 Astronomical Observatory of Torino, Italy
J.E. Morrison
Affiliation:
2 Space Telescope Science Institute, USA
B.J. McLean
Affiliation:
2 Space Telescope Science Institute, USA
C.R. Sturch
Affiliation:
2 Space Telescope Science Institute, USA 3 Computer Science Corporation at STScI

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We present a first attempt to compute an astrometric solution of POSS-IIplates using TYCHO stars as the reference catalogue. Also, we have made use of a special catalogue of stars observed with the Carlsberg Meridian Circlein La Palma between 1994 and 1995, brought into the HIPPARCOS reference system. Such a catalogue consists of a double strip along the equator, fairly dense (approximately 10 stars per square degree), faint (average magnitude 12.5), with an average error at epoch of ~ 150 mas per coordinate. Since the limiting magnitude of TYCHO stars is about 11.5, almost exactly one magnitude less than the CAMC special catalogues’ average, the latter has served as a very useful external comparison, although a more interesting magnitude range would have been 14-15. In this respect, we note that the Schmidt plates under study cover a large area (6.4 x 6.4 degree) and have fairly long exposures (~ 60 min); therefore, a possible magnitude dependence of the model needs to be carefully investigated. The results shown in the table above, which were obtained using a 2nd order polynomial in conjunction with a mask method using 5 plates only are very promising. The average external error over the entire plate area is about 0.2 arsecper coordinate, after the CAMC error have been subtracted.

Type
II. Joint Discussions
Copyright
Copyright © Kluwer 1998