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J/MNRAS/417/2230 BVRI+SDSS+2MASS and WISE photometry of 289 stars (Bilir+, 2011)

Transformations between the WISE, 2MASS, SDSS and BVRI photometric systems. I. Transformation equations for dwarfs. Bilir S., Karaali S., Ak S., Dagtekin N.D., Onal O., Yaz E., Coskunoglu B., Cabrera-Lavers A. <Mon. Not. R. Astron. Soc., 417, 2230-2238 (2011)> =2011MNRAS.417.2230B
ADC_Keywords: Surveys ; Photometry, infrared Keywords: techniques: photometric - catalogues - surveys Abstract: We present colour transformations for the conversion of the W1 and W2 magnitudes of the Wide-field Infrared Survey Explorer (WISE) photometric system to the Johnson-Cousins BVRI, Sloan Digital Sky Survey gri and Two-Micron All-Sky Survey JHKs photometric systems, for dwarfs. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 111 289 Johnson-Cousins, SDSS, 2MASS and WISE magnitudes and colours of the sample stars
See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) II/311 : WISE All-Sky Data Release (Cutri+ 2012) J/MNRAS/384/1178 : 2MASS, SDSS and BVRI photometry for 825 stars (Bilir+, 2008) : SDSS Home Page Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 14 A14 --- [BAK2008] Star name, from Bilir et al. 2008, Cat. J/MNRAS/384/1178 16- 24 F9.5 deg GLON Galactic longitude 26- 33 F8.5 deg GLAT Galactic latitude 35- 40 F6.3 mag Vmag ?=- Johnson V apparent magnitude 42- 46 F5.3 mag B-V ?=- Johnson B-V colour index 48- 52 F5.3 mag R-I ?=- Cousins R-I colour index 54- 59 F6.3 mag gmag SDSS g apparent magnitude 61- 65 F5.3 mag g-r SDSS g-r colour index 67- 71 F5.3 mag r-i SDSS r-i colour index 73- 78 F6.3 mag Jmag 2MASS J apparent magnitude 80- 84 F5.3 mag J-H 2MASS J-H colour index 86- 91 F6.3 mag H-Ks 2MASS H-Ks colour index 93- 98 F6.3 mag W1mag Wise W1 apparent magnitude 100-105 F6.3 mag W1-W2 Wise W1-W2 colour index 107-111 F5.3 mag E(B-V) Reduced E(B-V) colour excess
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 18-May-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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