Measuring Dust with Pan-STARRs

Details Measuring Dust with Pan-STARRs Measuring Dust with Pan-STARRs

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21832107f&link_type=abstract

American Astronomical Society, AAS Meeting #218, #321.07; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The colors of main sequence turnoff stars may be used to measure the
reddening of the stars by foreground dust. Using Pan-STARRs 3 pi data,
we have derived reddenings over a large part of the sky. I will show how
these reddening measurements can be used as a calibration check of the
PS1 data, and a test of the SFD (1998) dust map.

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