Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.237p..21m&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 237, March 1, 1989, p. 21P-26P.
Astronomy and Astrophysics
Astronomy
23
Astronomical Photometry, Stellar Spectra, Supernova 1987A, Ubv Spectra, Emission Spectra, Line Spectra
Scientific paper
The response functions of the VRI pass-bands in use at CTIO and at SAAO can be reconstructed from the color transformations to the standard system. The CTIO I-band is found to have a much bluer long-wavelength cut-off than does the one used at SAAO. In consequence, the Ca II 8600A emission lines, which are very strong in the spectrum of SN1987A, are included in the I measurement at SAAO but are excluded from the CTIO photometry. This is the probable reason for the disagreement of up to 0.3 mag between the values for I(c) obtained at the two observatories.
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