Magellanic clouds ultraviolet observations : J/AJ/116/180

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Authors : Parker J.W. orcid , Hill J.K., Cornett R.H. (hide) , Hill J.K., Cornett R.H. et..al

VizieR DOI : 10.26093/cds/vizier.51160180
Bibcode : 1998AJ....116..180P (ADS) (Simbad) (Objects)
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CDS Keywords : Magellanic Clouds; Photometry, ultraviolet
UAT : Magellanic Clouds, Ultraviolet photometry

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Inserted into VizieR : 18-Feb-1999
Last modification : 06-Apr-2023

Ultraviolet Imaging Telescope observations of the Magellanic clouds (1998)

Keywords : Magellanic Clouds - open clusters and associations general - stars: early-type - stars: luminosity function, mass function - ultraviolet emission

Abstract:The catalog is derived from wide-field far-ultraviolet (FUV; 1300-1800{AA}) images of the Large and Small Magellanic Clouds (LMC, SMC) obtained by the Ultraviolet Imaging Telescope (UIT) during the Astro-1 (1990 December 1-10) and Astro-2 (1995 March 2-18) missions. The FUV magnitudes are derived from point-spread function photometry for 37,333 stars in the LMC (the UIT FUV magnitudes for 11,306 stars in the SMC were presented by Cornett et al. (1997AJ....113.1011C), with a completeness limit of m_UV_ ~ 15mag and a detection limit of m_UV_ ~ 17.5. The average uncertainty in the photometry is ~ 0.1mag. ...(more)
Abstract: (hide)
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The catalog is derived from wide-field far-ultraviolet (FUV; 1300-1800{AA}) images of the Large and Small Magellanic Clouds (LMC, SMC) obtained by the Ultraviolet Imaging Telescope (UIT) during the Astro-1 (1990 December 1-10) and Astro-2 (1995 March 2-18) missions. The FUV magnitudes are derived from point-spread function photometry for 37,333 stars in the LMC (the UIT FUV magnitudes for 11,306 stars in the SMC were presented by Cornett et al. (1997AJ....113.1011C), with a completeness limit of m_UV_ ~ 15mag and a detection limit of m_UV_ ~ 17.5. The average uncertainty in the photometry is ~ 0.1mag. 


                


                

                    

                


                

                    

                


                

                    
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