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J/PASJ/61/177       15um AKARI observations in CDFS field    (Burgarella+, 2009)

Deep 15um AKARI observations in the CDFS: Estimating dust luminosities for a MIR-selected sample and for Lyman Break Galaxies and the evolution of Ldust/LUV with the redshift. Burgarella D., Buat V., Takeuchi T.T., Wada T., Pearson C. <Publ. Astron. Soc. Jap., 61, 177-192 (2009)> =2009PASJ...61..177B
ADC_Keywords: Galaxy catalogs ; Redshifts ; Infrared sources Keywords: cosmology: observations - galaxies: evolution - galaxies: formation - galaxies: high redshift - infrared: galaxies Abstract: Deep observations of the Chandra Deep Field South have been secured at 15um with AKARI/IRC infrared space telescope. From these observations, we define a sample of mid infrared-selected galaxies at 15um and we also obtain 15um flux densities for a sample of Lyman Break Galaxies at z∼1 already observed at 24um with Spitzer/MIPS. Description: The AKARI satellite is a Japanese space mission dedicated to infrared astrophysics and was launched on board JAXA's M-V8 Launch Vehicle on 2006 February 22 Japan Standard Time, JST. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 71 239 15um-selected sample table3.dat 71 27 z∼1 Lyman break galaxy sample
See also: II/253 : Chandra Deep Field South: multi-colour data (Wolf+, 2008) J/A+A/384/81 : ESO Imaging Survey. CDFS point sources (Hatziminaoglou+, 2002) J/A+A/403/493 : Chandra Deep Field South H-band observation (Moy+, 2003) J/A+A/465/1099 : Redshift catalog of 691 objects in CDFS (Ravikumar+, 2007) J/ApJS/179/19 : CDFS survey: 2 Ms source catalogs (Luo+, 2008) Byte-by-byte Description of file: table2.dat table3.dat
Bytes Format Units Label Explanations
1- 5 I5 --- COMBO17 COMBO 17 identification number, [WDK2001] NNNNN in Simbad 7- 15 F9.6 deg RAdeg Right ascension in decimal degrees (J2000) 17- 26 F10.6 deg DEdeg Declination in decimal degrees (J2000) 28- 34 F7.3 --- z ?=-99.000 Redshift (from COMBO 17 database) 36- 43 F8.3 uJy S15um AKARI flux density at 15um 45- 50 F6.3 uJy e_S15um rms uncertainty on S15um 52- 57 F6.4 mJy S24um ?=- Spitzer flux density at 24um 59- 64 F6.4 mJy e_S24um ?=- rms uncertainty on S24um 66- 71 F6.3 [solLum] logLdust ?=- Dust luminosity (1)
Note (1): Dust luminosities estimated from the 24 micrometer flux densities using Takeuchi et al. (2005A&A...432..423T).
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 23-Nov-2009
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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