The Magellanic Clouds Photometric Survey: the Small Magellanic Cloud Stellar Catalog and Extinction Map
نویسندگان
چکیده
We present our catalog of U , B, V , and I stellar photometry of the central 18 sq.◦ area of the Small Magellanic Cloud. We combine our data with the 2MASS and 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 I from the microlensing database of OGLE and I 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 investigate the nature of extinction as a function of stellar population. Subject headings: Magellanic Clouds — galaxies: photometry — galaxies: stellar content — dust,extinction — catalogs
منابع مشابه
The Magellanic Clouds Photometric Survey: the Large Magellanic Cloud Stellar Catalog and Extinction Map
We present our catalog of U , B, V , and I stellar photometry of the central 64 deg area of the Large Magellanic Cloud. Internal and external astrometric and photometric tests using existing optical photometry (U , B, and V from Massey’s bright star catalog and I from the near-infrared sky survey DENIS) are used to confirm our observational uncertainty estimates. We fit stellar atmosphere model...
متن کاملA Digital Photometric Survey of the Magellanic Clouds: First Results From One Million Stars
We present the first results from, and a complete description of, our ongoing UBV I digital photometric survey of the Magellanic Clouds. In particular, we discuss the photometric quality and automated reduction of a CCD survey (magnitude limits, completeness, and astrometric accuracy) that covers the central 8 × 8 of the Large Magellanic Cloud (LMC) and 4 × 4 of the Small Magellanic Cloud (SMC)...
متن کاملCharacteristic Scales in Stellar Clustering: A Transition Near the Disk Scale Height
The autocorrelation function provides an objective test for the existence of special scales in the hierarchical clustering of young stars. We apply this measure to single-star photometry for the brightest main sequence stars in the Small Magellanic Cloud (SMC), the Large Magellanic Cloud (LMC), M33, and M31, using data from the Magellanic Clouds Photometric Survey and the Massey Local Group Sur...
متن کاملThe Star Clusters of the Small Magellanic Cloud: Age Distribution
We present age measurements for 195 star clusters in the Small Magellanic Cloud based on comparison of integrated colors measured from the Magellanic Clouds Photometric Survey with models of simple stellar populations. We find that the modeled nonuniform changes of cluster colors with age can lead to spurious age peaks in the cluster age distribution, that the observed numbers of clusters with ...
متن کاملDust and Stellar Populations in the Large Magellanic Cloud
We present an analysis of line-of-sight extinction measurements obtained using data from the Magellanic Clouds Photometric Survey (Zaritsky, Harris, & Thompson 1997, AJ, 114, 1002), which provides 4-filter photometry for millions of stars in the Large Magellanic Cloud. We find that visual extinctions are typically larger by several tenths of a magnitude for stars with effective temperatures > 1...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008