Stellar Distribution Near SA 127, SA 141, SA 189 (Ratnatunga 1983)

Details Stellar Distribution Near SA 127, SA 141, SA 189 (Ratnatunga 1983) Stellar Distribution Near SA 127, SA 141, SA 189 (Ratnatunga 1983)

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat.2121....0r&link_type=abstract

VizieR On-line Data Catalog: II/121. Originally published in: Ph.D. Dissertation, The Australian National University, Canberra

Computer Science

Selected Areas: Stellar Distribution

Scientific paper

Photographic photometry and 1950 coordinates were determined using Automated Image location on 50 micron aperture PDS scans of the regions on UKSTU Schmidt plates. Galaxy contamination, which is small at these relatively bright apparent magnitudes, has not been removed from the images located. The image locating algorithm does not locate faint stars within 9 seconds of arc of an image of a brighter star on the plate. Assuming uniform random distributions, the estimated incompleteness is 0.5% at magnitude 15 and 2.2% at 17.5. (3 data files).

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