TY - JOUR
T1 - The magellanic clouds photomtric survey
T2 - The small magellanic cloud stellar catalog and extinction map
AU - Zaritsky, Dennis
AU - Harris, Jason
AU - Thompson, Ian B.
AU - Grebel, Eva K.
AU - Massey, Philip
N1 - Copyright:
Copyright 2004 Elsevier Science B.V., Amsterdam. All rights reserved.
PY - 2002/2
Y1 - 2002/2
N2 - We present our catalog of U, B, V, and I stellar photometry of the central 18 deg2 area of the Small Magellanic Cloud. We combine our data with the Two Micron All Sky Survey and Deep Near-Infrared Southern Sky Survey (DENIS) catalogs to provide, when available, U through Ks data for stars. Internal and external astrometric and photometric tests using existing optical photometry (U, B, and V from Massey's bright star catalog; B, V, and 7 from the microlensing database of OGLE; and 7 from the near-infrared sky survey DENIS) are used to determine the observational uncertainties and identify systematic errors. We fit stellar atmosphere models to the optical data to check the consistency of the photometry for individual stars across the passbands and to estimate the line-of-sight extinction. Finally, we use the estimated line-of-sight extinctions to produce an extinction map across the Small Magellanic Cloud, and we investigate the nature of extinction as a function of stellar population.
AB - We present our catalog of U, B, V, and I stellar photometry of the central 18 deg2 area of the Small Magellanic Cloud. We combine our data with the Two Micron All Sky Survey and Deep Near-Infrared Southern Sky Survey (DENIS) catalogs to provide, when available, U through Ks data for stars. Internal and external astrometric and photometric tests using existing optical photometry (U, B, and V from Massey's bright star catalog; B, V, and 7 from the microlensing database of OGLE; and 7 from the near-infrared sky survey DENIS) are used to determine the observational uncertainties and identify systematic errors. We fit stellar atmosphere models to the optical data to check the consistency of the photometry for individual stars across the passbands and to estimate the line-of-sight extinction. Finally, we use the estimated line-of-sight extinctions to produce an extinction map across the Small Magellanic Cloud, and we investigate the nature of extinction as a function of stellar population.
KW - Catalogs
KW - Dust, extinction
KW - Galaxies: photometry
KW - Galaxies: stellar content
KW - Magellanic Clouds
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U2 - 10.1086/338437
DO - 10.1086/338437
M3 - Review article
AN - SCOPUS:0001007455
VL - 123
SP - 855
EP - 872
JO - Astronomical Journal
JF - Astronomical Journal
SN - 0004-6256
IS - 2 1754
ER -