We derive an intrinsic colour calibration for F–K stars using broad band Johnson colours and line indices KP and $HP2$. Through this calibration we can determine $E(B-V)$ of an individual star within 0.03 mag. The $E(B-V)$ values thus derived are in excellent agreement with those derived from Strömgren photometry through the Schuster & Nissen (1989) calibration. The agreement is also good with the reddening maps of Burstein & Heiles (1982) and Schlegel et al. (1998), although in this case there exists a small offset of about 0.01 mag. This calibration may be applied to the large body of data of the HK survey extension which will be published in the near future
Although the use of RGB photometry has exploded in the last decades due to the advent of high-qualit...
Context.With the $\Delta a$ photometric system, it is possible to study very distant galactic and ev...
We establish an empirical effective temperature calibration of main sequence, luminosity class V to ...
We derive an intrinsic colour calibration for F--K stars using broad band Johnson colours and line i...
In recent years, several authors have revised the calibrations used to compute physical parameters (...
Context. With the ?a photometric system, it is possible to study very distant galactic and even extr...
A calibration of color indices of the Strömvil photometric system in terms of physical parameters of...
We have used recent Kurucz models and numerous standard stars to improve the calibration of the Gene...
With the Delta a photometric system, it is possible to study very distant galactic and even extragal...
Aims. The surface brightness-colour relation (SBCR) is a basic tool for establishing precise and acc...
Context. Gaia Data Release 1 allows the recalibration of standard candles such as the red clump star...
A collection of Johnson/Cousins photometry for stars with known [Fe/H] is used to generate color-col...
Context. The use of model atmospheres for deriving stellar fundamental parameters, such as Teff, l...
. In recent years, several authors have revised the calibrations used to compute physical parameter...
Intrinsic infrared colors of stars in the Johnson 11 color system are derived. The database is a lis...
Although the use of RGB photometry has exploded in the last decades due to the advent of high-qualit...
Context.With the $\Delta a$ photometric system, it is possible to study very distant galactic and ev...
We establish an empirical effective temperature calibration of main sequence, luminosity class V to ...
We derive an intrinsic colour calibration for F--K stars using broad band Johnson colours and line i...
In recent years, several authors have revised the calibrations used to compute physical parameters (...
Context. With the ?a photometric system, it is possible to study very distant galactic and even extr...
A calibration of color indices of the Strömvil photometric system in terms of physical parameters of...
We have used recent Kurucz models and numerous standard stars to improve the calibration of the Gene...
With the Delta a photometric system, it is possible to study very distant galactic and even extragal...
Aims. The surface brightness-colour relation (SBCR) is a basic tool for establishing precise and acc...
Context. Gaia Data Release 1 allows the recalibration of standard candles such as the red clump star...
A collection of Johnson/Cousins photometry for stars with known [Fe/H] is used to generate color-col...
Context. The use of model atmospheres for deriving stellar fundamental parameters, such as Teff, l...
. In recent years, several authors have revised the calibrations used to compute physical parameter...
Intrinsic infrared colors of stars in the Johnson 11 color system are derived. The database is a lis...
Although the use of RGB photometry has exploded in the last decades due to the advent of high-qualit...
Context.With the $\Delta a$ photometric system, it is possible to study very distant galactic and ev...
We establish an empirical effective temperature calibration of main sequence, luminosity class V to ...