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J/A+A/528/A107  GALEX Ultraviolet Virgo Cluster Survey (GUViCS) (Boselli+, 2011)

The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). I. The UV luminosity function of the central 12 sq. deg. Boselli A., Boissier S., Heinis S., Cortese L., Ilbert O., Hughes T., Cucciati O., Davies J., Ferrarese L., Giovanelli R., Haynes M.P., Baes M., Balkowski C., Brosch N., Chapman S.C., Charmandaris V., Clemens M.S., Dariush A., De Looze I., Di Serego Alighieri S., Duc P.-A., Durrell P.R., Emsellem E., Erben T., Fritz J., Garcia-Appadoo D.A., Gavazzi G., Grossi M., Jordan A., Hess K.M., Huertas-Company M., Hunt L.K., Kent B.R., Lambas D.G., Lancon A., MacArthur L.A., Madden S.C., Magrini L., Mei S., Momjian E., Olowin R.P., Papastergis E., Smith M.W.L., Solanes J.M., Spector O., Spekkens K., Taylor J.E., Valotto C., Van Driel W., Verstappen J., Vlahakis C., Vollmer B., Xilouris E.M. <Astron. Astrophys., 528, A107 (2011)> =2011A&A...528A.107B
ADC_Keywords: Clusters, galaxy ; Ultraviolet Keywords: galaxies: clusters: individual: Virgo - galaxies: evolution - galaxies: fundamental parameters - ultraviolet: galaxies - galaxies: luminosity function, mass function Abstract: The GALEX Ultraviolet Virgo Cluster Survey (GUViCS) is a complete blind survey of the Virgo cluster covering ∼40 sq. deg in the far UV (FUV, λeff=1539Å, Δλ=442Å) and ∼120 sq. deg in the near UV (NUV, λeff=2316Å, Δλ=1060Å). The goal of the survey is to study the ultraviolet (UV) properties of galaxies in a rich cluster environment, spanning a wide luminosity range from giants to dwarfs, and regardless of prior knowledge of their star formation activity. The UV data will be combined with those in other bands (optical: NGVS; far-infrared - submm: HeViCS; HI: ALFALFA) and with our multizone chemo-spectrophotometric models of galaxy evolution to make a complete and exhaustive study of the effects of the environment on the evolution of galaxies in high density regions. We present here the scientific objectives of the survey, describing the observing strategy and briefly discussing different data reduction techniques. Using UV data already in-hand for the central 12 sq. deg we determine the FUV and NUV luminosity functions of the Virgo cluster core for all cluster members and separately for early- and late-type galaxies and compare it to the one obtained in the field and other nearby clusters (Coma, A1367). This analysis shows that the FUV and NUV luminosity functions of the core of the Virgo clusters are flatter (alpha~-1.1) than those determined in Coma and A1367. We discuss the possible origin of this difference. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 69 237 GALEX observations of the Virgo cluster region
See also: J/A+AS/41/421 : 1.4GHz survey in the Virgo region (Kotanyi 1980) J/A+A/418/1 : Virgo cluster region radio continuum spectra (Vollmer+, 2004) J/AJ/133/2569 : Arecibo legacy fast ALFA survey III. (Giovanelli+, 2007) J/AJ/135/588 : Arecibo legacy fast ALFA survey V. (Saintonge+, 2008) J/AJ/136/713 : Arecibo legacy fast ALFA survey. VI. (Kent+, 2008) J/ApJS/183/214 : Arecibo Legacy Fast Alfa Survey VIII. (Martin+, 2009) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 29 A29 --- Field Field name 31- 32 I2 h RAh Right ascension (J2000) 34- 35 I2 min RAm Right ascension (J2000) 37- 41 F5.2 s RAs Right ascension (J2000) 43 A1 --- DE- Declination sign (J2000) 44- 45 I2 deg DEd Declination (J2000) 47- 48 I2 arcmin DEm Declination (J2000) 50- 53 F4.1 arcsec DEs Declination (J2000) 55- 61 F7.1 s TNUV Near-UV (231nm) integration time 63- 69 F7.1 s TFUV ?=- Far-UV (153nm) UV integration time
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 18-Aug-2011
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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