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J/MNRAS/399/323    Simulated UVEX colors with reddening      (Groot+, 2009)

The UV-excess survey of the northern galactic plane. Groot P.J., Verbeek K., Greimel R., Irwin M., Gonzalez-Solares E., Gansicke B.T., De Groot E., Drew J., Augusteijn T., Aungwerojwit A., Barlow M., Barros S., van den Besselaar E.J.M., Casares J., Corradi R., Corral-Santana J.M., Deacon N., van Ham W., Hu H., Heber U., Jonker P.G., King R., Knigge C., Mampaso A., Marsh T.R., Morales-Rueda L., Napiwotzki R., Naylor T., Nelemans G., Oosting T., Pyrzas S., Pretorius M., Rodriguez-Gil P., Roelofs G.H.A., Sale S., Schellart P., Steeghs D., Szyszka C., Unruh Y., Walton N.A., Weston S., Witham A., Woudt P., Zijlstra A. <Mon. Not. R. Astron. Soc., 399, 323-339 (2009)> =2009MNRAS.399..323G
ADC_Keywords: Models ; Reddening ; Ultraviolet ; Galactic plane Keywords: surveys - stars: general - ISM: general - Galaxy: disc - Galaxy: stellar content - Galaxy: structure Abstract: The UV-Excess survey of the northern Galactic plane images a 10°x185° wide band, centred on the Galactic equator using the 2.5-m Isaac Newton Telescope in four bands (U, g, r, HeI 5875) down to ∼21-22mag (∼20 in HeI 5875). The setup and data reduction procedures are described. Simulations of the colours of main-sequence stars, giant, supergiants, DA and DB white dwarfs and AM Canum Venaticorum stars are made, including the effects of reddening. A first look at the data of the survey (currently 30 per cent complete) is given. Description: To interpret the UVEX observations, simulations of the colours of stars and the effect of reddening are a very powerful and important tool. In obtaining the simulated colours, we follow the procedure as outlined in Drew et al. (2005MNRAS.362..753D) for the IPHAS. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 101 34 UVEX colour indices for Pickles main-sequence stars including reddening tablea2.dat 101 27 UVEX colour indices for Pickles giants including reddening tablea3.dat 101 18 UVEX/IPHAS colour indices for Pickles supergiants including reddening tablea4.dat 180 40 UVEX/IPHAS colour indices for log(g)=8.0 Bergeron DA white dwarfs including reddening tablea5.dat 180 30 UVEX/IPHAS colour indices for log(g)=8.0 Koester DA white dwarfs including reddening tablea6.dat 180 19 UVEX/IPHAS colour indices for log(g)=8.0 Koester DB white dwarfs including reddening
Byte-by-byte Description of file: tablea[123].dat
Bytes Format Units Label Explanations
1- 7 A7 -- SpType Spectral type 9- 14 F6.3 mag U-g:0 U-g colour index for E(B-V)=0.0 16- 21 F6.3 mag g-r:0 g-r colour index for E(B-V)=0.0 23- 28 F6.3 mag HeI-r:0 HeI-r colour index for E(B-V)=0.0 (G1) 30- 35 F6.3 mag U-g:1 U-g colour index for E(B-V)=1.0 37- 41 F5.3 mag g-r:1 g-r colour index for E(B-V)=1.0 43- 47 F5.3 mag HeI-r:1 HeI-r colour index for E(B-V)=1.0 (G1) 49- 53 F5.3 mag U-g:2 U-g colour index for E(B-V)=2.0 55- 59 F5.3 mag g-r:2 g-r colour index for E(B-V)=2.0 61- 65 F5.3 mag HeI-r:2 HeI-r colour index for E(B-V)=2.0 (G1) 67- 71 F5.3 mag U-g:3 U-g colour index for E(B-V)=3.0 73- 77 F5.3 mag g-r:3 g-r colour index for E(B-V)=3.0 79- 83 F5.3 mag HeI-r:3 HeI-r colour index for E(B-V)=3.0 (G1) 85- 89 F5.3 mag U-g:4 U-g colour index for E(B-V)=4.0 91- 95 F5.3 mag g-r:4 g-r colour index for E(B-V)=4.0 97-101 F5.3 mag HeI-r:4 HeI-r colour index for E(B-V)=4.0 (G1)
Byte-by-byte Description of file: tablea4.dat tablea5.dat tablea6.dat
Bytes Format Units Label Explanations
1- 5 I5 K T Temperature 7- 12 F6.3 mag U-g:0 U-g colour index for E(B-V)=0.0 14- 19 F6.3 mag g-r:0 g-r colour index for E(B-V)=0.0 21- 26 F6.3 mag HeI-r:0 HeI-r colour index for E(B-V)=0.0 (G1) 28- 33 F6.3 mag r-Ha:0 r-Halpha colour index for E(B-V)=0.0 (G1) 35- 40 F6.3 mag r-i:0 r-i colur index for E(B-V)=0.0 42- 47 F6.3 mag U-g:1 U-g colour index for E(B-V)=1.0 49- 54 F6.3 mag g-r:1 g-r colour index for E(B-V)=1.0 56- 61 F6.3 mag HeI-r:1 HeI-r colour index for E(B-V)=1.0 (G1) 63- 68 F6.3 mag r-Ha:1 r-Halpha colour index for E(B-V)=1.0 (G1) 70- 75 F6.3 mag r-i:1 r-i colur index for E(B-V)=1.0 77- 82 F6.3 mag U-g:2 U-g colour index for E(B-V)=2.0 84- 89 F6.3 mag g-r:2 g-r colour index for E(B-V)=2.0 91- 96 F6.3 mag HeI-r:2 HeI-r colour index for E(B-V)=2.0 (G1) 98-103 F6.3 mag r-Ha:2 r-Halpha colour index for E(B-V)=2.0 (G1) 105-110 F6.3 mag r-i:2 r-i colur index for E(B-V)=2.0 112-117 F6.3 mag U-g:3 U-g colour index for E(B-V)=3.0 119-124 F6.3 mag g-r:3 g-r colour index for E(B-V)=3.0 126-131 F6.3 mag HeI-r:3 HeI-r colour index for E(B-V)=3.0 (G1) 133-138 F6.3 mag r-Ha:3 r-Halpha colour index for E(B-V)=3.0 (G1) 140-145 F6.3 mag r-i:3 r-i colur index for E(B-V)=3.0 147-152 F6.3 mag U-g:4 U-g colour index for E(B-V)=4.0 154-159 F6.3 mag g-r:4 g-r colour index for E(B-V)=4.0 161-166 F6.3 mag HeI-r:4 HeI-r colour index for E(B-V)=4.0 (G1) 168-173 F6.3 mag r-Ha:4 r-Halpha colour index for E(B-V)=4.0 (G1) 175-180 F6.3 mag r-i:4 r-i colur index for E(B-V)=4.0
Global Notes: Note (G1): narrow-band filters: -------------------------------------- HeI 587.5nm ±4.0nm (FWHM) Ha 656.8nm ±9.5nm (FWHM) --------------------------------------
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 08-Mar-2010
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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