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The Shane-Wirtanen counts - Systematics and two-point correlation functionResidual errors in the Selder et al. (SSGP) map which caused a break in both the correlation factor (CF) and the filamentary appearance of the Shane-Wirtanen map are examined. These errors, causing a residual rms fluctuation of 11 percent in the SSGP-corrected counts and a systematic rms offset of 8 percent in the mean count per plate, can be attributed to counting pattern and plate vignetting. Techniques for CF reconstruction in catalogs affected by plate-related systematic biases are examined, and it is concluded that accurate restoration may not be possible. Surveys designed to measure the CF at the depth of the SW counts on a scale of 2.5 deg, must have systematic errors of less than or about 0.04 mag.
Document ID
19860055090
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
De Lapparent, V.
(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; Ecole Normale Superieure de Jeunes Filles; Paris VII, Universite Paris, France)
Kurtz, M. J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Geller, M. J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
May 15, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 304
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
86A39828
Funding Number(s)
CONTRACT_GRANT: NAGW-201
Distribution Limits
Public
Copyright
Other

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