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J/MNRAS/412/127  ACCESS. II. Shapley galaxies FUV-FIR photometry (Haines+, 2011)

ACCESS. II. A complete census of star formation in the Shapley supercluster - UV and IR luminosity functions. Haines C.P., Busarello G., Merluzzi P., Smith R.J., Raychaudhury S., Mercurio A., Smith G.P. <Mon. Not. R. Astron. Soc., 412, 127-144 (2011)> =2011MNRAS.412..127H (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy; Galaxies, photometry; Photometry, ultraviolet; Photometry, UBVRI; Photometry, millimetric/submm Keywords: galaxies: clusters: general - galaxies: clusters: individual A3556 - galaxies: clusters: individual A3558 - galaxies: clusters: individual A3562 - galaxies: evolution - galaxies: stellar content Abstract: We present panoramic Spitzer/MIPS mid- and far-infrared (MIR/FIR) and GALEX ultraviolet imaging of the most massive and dynamically active system in the local Universe, the Shapley supercluster at z=0.048, covering the five clusters that make up the supercluster core. We combine these data with existing spectroscopic data from 814 confirmed supercluster members to produce the first study of a local rich cluster including both ultraviolet and infrared luminosity functions (LFs). Description: The ultraviolet and mid-infrared data analysed in this paper are complemented by existing panoramic optical B- and R-band imaging from the Shapley Optical Survey (SOS: Haines et al. 2006MNRAS.371...55H; Mercurio et al. 2006MNRAS.368..109M) and near-infrared K-band imaging (Merluzzi et al. 2010MNRAS.402..753M, Paper I) The UV data analysed in this paper consist of four contiguous GALEX pointings making up the Cycle 4 Guest Investigation proposal GI4-098 (P.I. R.J. Smith), and which were observed in 2008 May. The panoramic Spitzer mid-infrared observations of the Shapley supercluster core were carried out over 2008 August 27-30 within the Cycle 5 GO programme 50510 (PI: C.P. Haines). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 93 863 FUV-FIR photometry for spectroscopic members of the Shapley supercluster (10700<Vel(km/s)<17000)
See also: : ACCESS Home Page Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh Right ascension (J2000) 4- 5 I2 min RAm Right ascension (J2000) 7- 12 F6.3 s RAs Right ascension (J2000) 14 A1 --- DE- Declination sign (J2000) 15- 16 I2 deg DEd Declination (J2000) 18- 19 I2 arcmin DEm Declination (J2000) 21- 25 F5.2 arcsec DEs Declination (J2000) 27- 31 I5 km/s HV Heliocentric recession velocity of the galaxy 33- 38 F6.3 mag Kmag ?=- UKIRT/WFCAM K-band total magnitude (Vega) 40- 45 F6.3 mag Rmag ?=- WFI R-band total magnitude (Vega) 47- 52 F6.3 mag B-R ?=- B-R colour within 17" diameter aperture 54- 59 F6.3 mag NUV ?=- GALEX NUV total magnitude (AB system) 61- 66 F6.3 mag FUV ?=- GALEX FUV total magnitude (AB system) 68- 73 F6.3 mJy F24 ?=- Spitzer/MIPS 24micron flux 75- 79 F5.3 mJy e_F24 ?=- Uncertainty in F24 81- 87 F7.2 mJy F70 ?=- Spitzer/MIPS 70micron flux 89- 93 F5.2 mJy e_F70 ?=- Uncertainty in F70
History: From electronic version of the journal References: Merluzzi et al., Paper I 2010MNRAS.402..753M
(End) Patricia Vannier [CDS] 12-Sep-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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