Near-infrared photometry of stars

Details Near-infrared photometry of stars Near-infrared photometry of stars

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...90..105l&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 90, no. 1, Oct. 1991, p. 105-108.

Astronomy and Astrophysics

Astrophysics

1

Infrared Photometry, Near Infrared Radiation, Stellar Magnitude, Stellar Spectrophotometry, Calibrating, Mira Variables, Stellar Color

Scientific paper

Results are presented of infrared photometric observations performed on comparison stars during a monitoring of long-period variables. These observations, spread over a lapse of about 5 years, are used to derive the J, H, and K magnitudes of 54 stars in the photometric system described by Koornneef (1983). The 1950.0 coordinates, spectral types, visual magnitudes, average magnitudes, and the number of observations are given for each object.

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