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Related papers: An Improved Metallicity Calibration with UBV Photo…

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Although core helium-burning red clump (RC) stars are faint at ultraviolet wavelengths, their ultraviolet-optical color is a unique and accessible probe of their physical properties. Using data from the GALEX All Sky Imaging Survey, Gaia…

Solar and Stellar Astrophysics · Physics 2019-02-20 Steven Mohammed , David Schiminovich , Keith Hawkins , Benjamin Johnson , Dun Wang , David W. Hogg

The calibrations linking observed luminosities to the star formation rate depend on the assumed stellar population synthesis model, initial mass function, star formation and metal enrichment history, and whether reprocessing by dust and gas…

Astrophysics of Galaxies · Physics 2019-10-23 Stephen M. Wilkins , Christopher C. Lovell , Elizabeth R. Stanway

The consistency of the metallicity distributions of F, G and K dwarfs is studied. We present a new metallicity distribution for K dwarfs using metallicities determined from uvby photometry. There is a remarkable paucity of metal-poor K…

Astrophysics · Physics 2007-05-23 H. J. Rocha-Pinto , W. J. Maciel

We derive a new relation between the metallicity of Seyfert 2 Active Galactic Nuclei (AGNs) and the intensity of the narrow emission-lines ratio $N2O2$=log([N II]$\lambda$6584/[O II]$\lambda$3727). The calibration of this relation was…

Astrophysics of Galaxies · Physics 2017-02-01 C. S. Castro , O. L. Dors , M. V. Cardaci , G. F. Hagele

(Abridged) We investigate the effect of metallicity calibrations, AGN classification, and aperture covering fraction on the local mass-metallicity (MZ) relation using 27,730 star-forming galaxies from the Sloan Digital Sky Survey (SDSS)…

Astrophysics · Physics 2014-11-18 Lisa J. Kewley , Sara L. Ellison

We present metallicity dependent transformation equations between UBV and SDSS ugr colours for red giants with synthetic data. The ranges of the colours used for the transformations are 0.400 $\leq(B-V)_{0}\leq$ 1.460, -0.085$\leq(U -…

Solar and Stellar Astrophysics · Physics 2015-06-16 Salih Karaali , Esma Yaz Gökçe

Aims. We present a continuation of our study about the relation between stellar mass and gas-phase metallicity in the VIMOS VLT Deep Survey (VVDS). In this work we extend the determination of metallicities up to redshift = 1.24 for a sample…

We present equivalent widths, improved model atmosphere parameters, and revised abundances for 14 species of 11 elements derived from high resolution optical spectroscopy of 311 metal-poor stars. All of these stars had their parameters…

Solar and Stellar Astrophysics · Physics 2025-02-27 Sanil Mittal , Ian U. Roederer

Based on the Sloan Digital Sky Survey (SDSS), we develop a new monte-carlo based method to estimate the photometric metallicity distribution function (MDF) for stars in the Milky Way. Compared with other photometric calibration methods,…

Astrophysics of Galaxies · Physics 2016-07-27 Jiayin Gu , Cuihua Du , Yingjie jing , Wenbo Zuo

We collect a sample of stars observed both in LAMOST and Gaia which have colors implying a temperature hotter than 7000 K. We train a machine learning algorithm on LAMOST spectroscopic data which has been tagged with stellar classifications…

Astrophysics of Galaxies · Physics 2021-05-12 John J. Vickers , Zhao-Yu Li , Martin C. Smith , Juntai Shen

The near-infrared Calcium II Triplet (CaT), around 850nm, is a key metallicity indicator for red giant stars. We present a revised [Fe/H] calibration as a function of CaT line strengths and four luminosity indicators, including the $Gaia$…

Solar and Stellar Astrophysics · Physics 2026-02-04 M. Navabi , R. Carrera , N. E. D. Noël , C. Gallart , E. Pancino , M. De Leo

We present an empirical calibration of the uvby-beta photometric system to determine the intrinsic colours and indices and the astrophysical parameters of the underlying star, valid for Be stars earlier than B5. The procedure allows the…

Astrophysics · Physics 2007-05-23 Juan Fabregat , Jose M. Torrejon

We derived two semi-empirical calibrations between the metallicity of the Narrow Line Region (NLR) of type-2 Active Galactic Nuclei and the rest-frame of the N V$\lambda$1240/He II$\lambda1640$, C43=log[(C IV$\lambda1549$+C…

Astrophysics of Galaxies · Physics 2019-05-15 O. L. Dors , A. F. Monteiro , M. V. Cardaci , G. F. Hagele , A. C. Krabbe

We establish an empirical effective temperature calibration of main sequence, luminosity class V to III B-type stars for the Delta a photometric system which was originally developed to detect magnetic chemically peculiar objects of the…

Astrophysics · Physics 2009-11-11 E. Paunzen , A. Schnell , H. M. Maitzen

Context. Precise and accurate determinations of effective temperature and surface gravity are mandatory to derive reliable chemical abundances and fundamental parameters like distances, masses, radii, luminosities of OB stars. Aims.…

Solar and Stellar Astrophysics · Physics 2015-06-12 Maria-Fernanda Nieva

We focus on an analysis of galaxies of high stellar mass and low metallicity. We cross-correlated the Millenium Galaxy Catalogue (MGC) and the Sloan Digital Sky Survey (SDSS) galaxy catalogue to provide a sample of MGC objects with high…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-20 M. S. Alonso , L. Michel-Dansac , D. G. Lambas

Using more than 100 galaxies in the MUSE Ultra Deep Field with spectroscopy from the Hubble Space Telescope's Wide Field Camera 3 and the Very Large Telescope's Multi Unit Spectroscopic Explorer, we extend the gas-phase mass-metallicity…

We present new accurate measurements of the physical properties of a statistically significant sample of 103 galaxies at z~2 using near-infrared spectroscopy taken as part of the 3D-HST survey. We derive redshifts, metallicities and star…

Cosmology and Nongalactic Astrophysics · Physics 2014-04-09 F. Cullen , M. Cirasuolo , R. J. McLure , J. S. Dunlop

We have begun developing a new metallicity calibration for RR Lyrae stars that includes high-temperature phase regions. Our calibration is an updated and expanded version of the Delta-S, equivalent width method, but which is applicable for…

Solar and Stellar Astrophysics · Physics 2013-10-03 E. Spalding , R. Wilhelm , N. De Lee

We present a re-analysis of the Geneva-Copenhagen survey, which benefits from the infrared flux method to improve the accuracy of the derived stellar effective temperatures and uses the latter to build a consistent and improved metallicity…