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Publications of the Astronomical Society of Australia
RESEARCH ARTICLE

Transformations from WISE to 2MASS, SDSS and BVI Photometric Systems: II. Transformation Equations for Red-Clump Stars

S. Bilir A E , S. Karaali A , N. D. Dağtekin A , Ö. Önal A , S. Ak A , T. Ak A and A. Cabrera-Lavers B C D
+ Author Affiliations
- Author Affiliations

A Istanbul University, Faculty of Sciences, Department of Astronomy and Space Sciences, 34119 University, Istanbul, Turkey

B Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain

C GTC Project Office, E-38205 La Laguna, Tenerife, Spain

D Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain

E Corresponding author. Email: sbilir@istanbul.edu.tr

Publications of the Astronomical Society of Australia 29(2) 121-131 https://doi.org/10.1071/AS11078
Submitted: 26 December 2011  Accepted: 2 February 2012   Published: 6 March 2012

Abstract

We present colour transformations for the conversion of Wide-Field Survey Explorer W1, W2, and W3 magnitudes to the Johnson–Cousins BVIc, Sloan Digital Sky Survey gri, and Two Micron All Sky Survey JHKs photometric systems, for red clump (RC) stars. RC stars were selected from the Third Radial Velocity Experiment Data Release. The apparent magnitudes were collected by matching the coordinates of this sample with different photometric catalogues. The final sample (355 RC stars) was used to obtain metallicity-dependent and free-of-metallicity transformations. These transformations combined with known absolute magnitudes at shorter wavelengths can be used in space density determinations for the Galactic (thin and thick) discs at distances larger than the ones evaluated with JHKs photometry alone, hence providing a powerful tool in the analysis of Galactic structure.

Keywords: techniques: photometric — catalogues — surveys


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