Near-infrared photometry of late-type stars with balloon-borne telescope

Details Near-infrared photometry of late-type stars with balloon-borne telescope Near-infrared photometry of late-type stars with balloon-borne telescope

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976tokab.245.2077k&link_type=abstract

Tokyo Astronomical Observatory, Tokyo Astronomical Bulletin, Second Series, no. 245, July 7, 1976, p. 2077-2080.

Astronomy and Astrophysics

Astronomy

3

Astronomical Photometry, Balloon-Borne Instruments, Infrared Astronomy, Infrared Photometry, Late Stars, Infrared Filters, Infrared Telescopes, Stellar Magnitude

Scientific paper

Balloon-borne observations were made from an altitude of 25 km approximately 120 km off the coast of northeastern Japan. The balloon then drifted westward across Japan island, taking near-infrared readings of late stars with a Reticon matrix camera as it went. Alpha-Aql was used as a reference for photometric comparison. Attention is given to observations of alpha-Boo, alpha-Sco, and alpha-Her.

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