B and V photometry of faint stars in the Large Magellanic Cloud

Details B and V photometry of faint stars in the Large Magellanic Cloud B and V photometry of faint stars in the Large Magellanic Cloud

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...73...37l&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 73, no. 1, April 1988, p. 37-50.

Astronomy and Astrophysics

Astrophysics

1

Faint Objects, Magellanic Clouds, Stellar Spectrophotometry, Visible Spectrum, Astronomical Catalogs, Electronography, Image Processing, Stellar Magnitude

Scientific paper

Photometric data on the Johnson BV system are given for 947 stars in a
field close to the bar of the Large Magellanic Cloud. The data have been
determined from electronographs calibrated through photoelectric
photometry. The visual magnitudes of the programme stars range from V =
14.63 to V = 23.13.

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