The visibility of two faint star sequences on the Palomar and ESO sky surveys

Details The visibility of two faint star sequences on the Palomar and ESO sky surveys The visibility of two faint star sequences on the Palomar and ESO sky surveys

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193..329w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Nov. 1980, p. 329-332. Research supported by the Australian Resear

Astronomy and Astrophysics

Astronomy

1

Electronography, Sky Surveys (Astronomy), Stellar Magnitude, Visual Observation, Astronomical Photography

Scientific paper

Stars with published electronographic B magnitudes fainter than the
accepted limiting magnitudes of both the Palomar and ESO B sky surveys
are clearly visible on both surveys. An independent estimate of the
magnitudes of these stars based on another deep sequence indicates a
possible inconsistency in the electronographic magnitudes.

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