A photometric sequence near SN 1987A

Details A photometric sequence near SN 1987A A photometric sequence near SN 1987A

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1253w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Oct. 1988, p. 1253-1255.

Astronomy and Astrophysics

Astronomy

1

Stellar Spectrophotometry, Supernova 1987A, Charge Coupled Devices, Stellar Luminosity, Stellar Magnitude

Scientific paper

CCD observations were obtained in March and November 1987 with the 0.9-m and 1.5-m CTIO telescopes in order to set up a photometric sequence near SN 1987A. The BVRI sequence consists of 18 stars with V magnitudes of between 9.8 and 16.8. The sequence can be used to calibrate photographic plates taken prior to the SN outburst in order to place limits on the magnitudes of the progenitor star of SN 1987A.

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