The Calibration of Absolute Magnitudes from Trigonometric Parallaxes - Sampling

Details The Calibration of Absolute Magnitudes from Trigonometric Parallaxes - Sampling The Calibration of Absolute Magnitudes from Trigonometric Parallaxes - Sampling

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf...41l&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Computer Science

13

Scientific paper

Methods for computing absolute magnitudes from small trigonometric
parallaxes are reviewed and discussed. It is demonstrated that a careful
examination of the sample space of observable (apparent magnitude,
parallax) is necessary for clarifying the difference - and overlap -
between magnitude limited and volume limited samples.

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