dc.contributor.author | Plevne, O. | |
dc.contributor.author | Ak, Serap | |
dc.contributor.author | Karaali, S. | |
dc.contributor.author | Ak, Tansel | |
dc.contributor.author | Bostanci, Z. F. | |
dc.contributor.author | Güçtekin, S. Tunçel | |
dc.contributor.author | Bilir, S. | |
dc.date.accessioned | 2021-03-04T12:58:02Z | |
dc.date.available | 2021-03-04T12:58:02Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | Güçtekin S. T. , Bilir S., Karaali S., Plevne O., Ak S., Ak T., Bostanci Z. F. , "Metallicity calibration and photometric parallax estimation: II. SDSS photometry", ASTROPHYSICS AND SPACE SCIENCE, cilt.362, sa.1, 2017 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.other | av_79ffef7c-1ef7-41cd-8453-9e4020f33ecf | |
dc.identifier.other | vv_1032021 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/83586 | |
dc.identifier.uri | https://doi.org/10.1007/s10509-016-2987-6 | |
dc.description.abstract | We used the updated [Fe/H] abundances of 168 F-G type dwarfs and calibrated them to a third order polynomial in terms of reduced ultraviolet excess, delta(0.41) defined with ugr data in the SDSS. We estimated the M-g absolute magnitudes for the same stars via the re-reduced Hipparcos parallaxes and calibrated the absolute magnitude offsets, Delta M-g, relative to the intrinsic sequence of Hyades to a third order polynomial in terms of delta(0.41). The ranges of the calibrations are -2 18 mag). | |
dc.language.iso | eng | |
dc.subject | Uzay bilimi | |
dc.subject | Temel Bilimler | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Fizik | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.title | Metallicity calibration and photometric parallax estimation: II. SDSS photometry | |
dc.type | Makale | |
dc.relation.journal | ASTROPHYSICS AND SPACE SCIENCE | |
dc.contributor.department | İstanbul Üniversitesi , Fen Bilimleri Enstitüsü , Fen Fakültesi Bölümü | |
dc.identifier.volume | 362 | |
dc.identifier.issue | 1 | |
dc.contributor.firstauthorID | 2210907 | |