Near-infrared energy distributions of M31

Details Near-infrared energy distributions of M31 Near-infrared energy distributions of M31

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978aj.....83.1377t&link_type=abstract

Astronomical Journal, vol. 83, Nov. 1978, p. 1377-1382.

Astronomy and Astrophysics

Astronomy

6

Andromeda Galaxy, Infrared Astronomy, Spectrophotometry, Calibrating, Error Analysis, Near Infrared Radiation, Wavelengths

Scientific paper

Spectrophotometric data obtained by comparing Spinrad-Taylor (1969) standards with Alpha Lyr are presented, along with a calibration of these data for wavelengths longward of 6000 A. M31 sky measurements made 1 deg south of the nucleus at five wavelengths between 6040 and 10,360 A, inclusive, are compared with near-IR spectrophotometry performed by Spinrad and Taylor (1971), Oke and Schwarzschild (1975), and O'Connell (1976). Agreement and discrepancies among the different data sets are discussed. Some possible explanations of the differences are discounted, and tests are performed which reveal no effects of error in mean extinction and brightness-dependent wavelength response.

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