Infrared space observatory photometry of circumstellar dust in Vega-type systems

Details Infrared space observatory photometry of circumstellar dust in Vega-type systems Infrared space observatory photometry of circumstellar dust in Vega-type systems

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998exdu.work..265f&link_type=abstract

Exozodiacal Dust Workshop, p. 265

Astronomy and Astrophysics

Astronomy

Main Sequence Stars, Stellar Envelopes, Astronomical Photometry, Calibrating, Infrared Space Observatory (Iso), Data Processing

Scientific paper

The ISOPHOT (Infrared Space Observatory Photometry) instrument onboard the Infrared Space Observatory (ISO) was used to obtain 3.6-90 micron photometry of Vega-type systems. Photometric data were calibrated with the ISOPHOT fine calibration source 1 (FCS1). Linear regression was used to derive transformations to make comparisons to ground-based and IRAS photometry systems possible. These transformations were applied to the photometry of 14 main-sequence stars. Details of these results are reported on.

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