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dc.contributor.authorKaraali, S
dc.contributor.authorBilir, S
dc.contributor.authorTuncel, S
dc.date.accessioned2021-03-05T09:28:25Z
dc.date.available2021-03-05T09:28:25Z
dc.date.issued2005
dc.identifier.citationKaraali S., Bilir S., Tuncel S., "New colour transformations for the sloan photometry, and revised metallicity calibration and equations for photometric parallax estimation", PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, cilt.22, ss.24-28, 2005
dc.identifier.issn1323-3580
dc.identifier.otherav_9dfd8013-f6f4-499e-b929-36b2becd7c57
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/106112
dc.identifier.urihttps://doi.org/10.1071/as04034
dc.description.abstractWe evaluated new colour transformations for the Sloan photometry by 224 standards and used them to revise both the equations for photometric parallax estimation and metallicity calibration cited by Karaali et al. ( 2003). This process improves the metallicity and absolute magnitude estimations by [Fe/H] less than or equal to 0.3 dex and M-g1(H) greater than or equal to 0.1 mag respectively. There is a high correlation for metallicities and absolute magnitudes derived for two systems, UBV and Sloan, by means of the revised calibrations.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleNew colour transformations for the sloan photometry, and revised metallicity calibration and equations for photometric parallax estimation
dc.typeMakale
dc.relation.journalPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
dc.contributor.department, ,
dc.identifier.volume22
dc.identifier.issue1
dc.identifier.startpage24
dc.identifier.endpage28
dc.contributor.firstauthorID173683


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