Photometric calibration of the APM Proper Motion Project

Details Photometric calibration of the APM Proper Motion Project Photometric calibration of the APM Proper Motion Project

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...78..249e&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 78, no. 2, May 1989, p. 249-268. Research supported by SERC.

Astronomy and Astrophysics

Astrophysics

24

Astronomical Photometry, Calibrating, Charge Coupled Devices, Stellar Magnitude, Astronomical Maps, Cameras, Color-Color Diagram, Southern Sky, Stellar Spectra, Tables (Data)

Scientific paper

Deep BVR photometry is presented in the magnitude range B = 11-21,
obtained using a CCD camera. These magnitudes are used to calibrate the
photographic photometry of the APM Proper Motion Project. Useful
color-color relationships are also presented, calculated using the
stellar spectra of Gunn and Stryker (1983).

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