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J/AJ/129/2074      Faint Chandra sources in SWIRE          (Franceschini+, 2005)

A complete multiwavelength characterization of faint Chandra X-ray sources seen in the Spitzer wide-area infrared extragalactic (SWIRE) survey. Franceschini A., Manners J., Polletta M.D.C., Lonsdale C., Gonzalez-Solares E., Surace J., Shupe D., Fang F., Xu C.K., Farrah D., Berta S., Rodighiero G., Perez-Fournon I., Hatziminaoglou E., Smith H.E., Siana B., Rowan-Robinson M., Nandra K., Babbedge T., Vaccari M., Oliver S., Wilkes B., Owen F., Padgett D., Frayer D., Jarrett T., Masci F., Stacey G., Almaini O., McMahon R., Johnson O., Lawrence A., Willott C. <Astron. J., 129, 2074-2101 (2005)> =2005AJ....129.2074F
ADC_Keywords: Galaxies, IR ; X-ray sources ; Active gal. nuclei Keywords: galaxies: evolution - quasars: general - X-rays: galaxies Abstract: We exploit deep combined observations with Spitzer and Chandra of the Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE) in the ELAIS N1 region to investigate the nature of the faint X-ray and IR sources in common, to identify active galactic nucleus (AGN)/starburst diagnostics, and to study the sources of the X-ray and IR cosmic backgrounds (XRB and CIRB). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 136 99 Relevant data on the Spitzer and Chandra source sample
See also: II/255 : SWIRE ELAIS N1 Source Catalogs (Surace+, 2004) J/MNRAS/343/293 : ELAIS deep X-ray survey. I. (Manners+, 2003) J/MNRAS/355/97 : Chandra/ELAIS mid-infrared sources (Manners+, 2004) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [MJA2003] Manners et al. (2003, Cat. J/MNRAS/343/293) identification number 5- 13 F9.5 deg RAdeg Right Ascension in decimal degrees (J2000) 15- 22 F8.5 deg DEdeg Declination in decimal degrees (J2000) 24- 29 F6.2 mJy S3.6um ? IRAC 3.6 micron flux density 31- 35 F5.3 mJy e_S3.6um ? Uncertainty in S3.6um 37- 42 F6.2 mJy S4.5um ? IRAC 4.5 micron flux density 44- 48 F5.3 mJy e_S4.5um ? Uncertainty in S4.5um 50- 55 F6.1 mJy S5.6um ? IRAC 5.6 micron flux density 57- 61 F5.2 mJy e_S5.6um ? Uncertainty in S5.6um 63- 69 F7.1 mJy S8um ? IRAC 8 micron flux density 71- 75 F5.2 mJy e_S8um ? Uncertainty in S8um 77- 84 F8.2 mJy S24um ? MIPS 24 micron flux density 86- 90 F5.2 mJy e_S24um ? Uncertainty in S24um 92- 95 F4.2 arcsec Dist Chandra to Spitzer angular distance 97-104 E8.2 mW/m2 SX Chandra (0.5-8keV) flux in erg/cm2/s 106-113 E8.2 mW/m2 e_SX Uncertainty in SX 115 I1 --- Type Type from the Optical/IR SED (1) 117-121 F5.2 --- HR X-ray hardness ratio (2) 123-126 F4.2 --- e_HR Uncertainty in HR 128-135 E8.3 10-7W XLum X-ray (0.5-8keV) luminosity in erg/s
Note (1): Type from the Optical/IR SED, defined as follows: 1 = type-1 AGN; 2 = type-2 AGN; 3 = galaxy; 4 = early-type galaxy. Note (2): HR=(H-S)/(H+S) where H and S are the background-subtracted X-ray counts in the hard (2.0-8.0keV) and soft (0.5-2.0keV) bands, respectively.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 07-Sep-2005
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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