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J/ApJ/642/126   Mid-IR observations in the extended Groth strip  (Barmby+, 2006)

Mid-infrared properties of X-ray sources in the extended Groth strip. Barmby P., Alonso-Herrero A., Donley J.L., Egami E., Fazio G.G., Georgakakis A., Huang J.-S., Laird E.S., Miyazaki S., Nandra K., Park S.Q., Perez-Gonzalez P.G., Rieke G.H., Rigby J.R., Willner S.P. <Astrophys. J., 642, 126-139 (2006)> =2006ApJ...642..126B
ADC_Keywords: Galaxies, IR ; X-ray sources Keywords: galaxies: active -- infrared: galaxies -- X-rays: galaxies Description: A sample of about 150 AGNs was selected from observations of Chandra and XMM X-ray observatories in a 300arcmin2 region of the extended Groth strip (EGS), and observed by the IRAC and MIPS instruments of the Spitzer IR telescope. About 68-80% of these sources were detected by Spitzer, and they show a wide range of mid-infrared properties. The IRAC SED type does not directly correspond to X-ray spectral type (hard/soft). The mid-IR properties of X-ray-detected Lyman break, radio, submillimeter, and optically faint sources vary widely, and for the most part are not distinct from those of the general X-ray/IR source population. X-ray sources emit 6-11% of the integrated mid-IR light, making them significant contributors to the cosmic infrared background. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 106 138 Infrared Properties of extended Groth strip (EGS) X-Ray Sources
See also: J/MNRAS/350/785 : XMM/CFDS catalogue (Waskett+, 2004) J/MNRAS/356/568 : Deep Chandra survey of the Groth Strip (Nandra+, 2005) J/ApJS/159/41 : DEEP Groth Strip Survey. I. (Vogt+, 2005) J/ApJS/142/1 : DEEP Groth Strip Survey. II. (Simard+, 2002) J/ApJ/599/1006 : DEEP Groth Strip Survey. VII. (Kobulnicky+, 2003) J/ApJS/157/175 : DEEP Groth Strip Survey. VIII. (Koo+, 2005) J/ApJ/571/136 : DEEP Groth Strip survey. X. (Im+, 2002) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- CXO ? Nandra et al. (2005MNRAS.360L..39N) source number (1) (2) 5- 7 I3 --- XMM ? Waskett et al. (2004, Cat. J/MNRAS/350/785) source number (1) (3) 9- 10 I2 h RAh Hour of Right Ascension (J2000) (4) 12- 13 I2 min RAm Minute of Right Ascension (J2000) (4) 15- 19 F5.2 s RAs Second of Right Ascension (J2000) (4) 21 A1 --- DE- Sign of the Declination (J2000) (4) 22- 23 I2 deg DEd Degree of Declination (J2000) (4) 25- 26 I2 arcmin DEm Arcminute of Declination (J2000) (4) 28- 31 F4.1 arcsec DEs Arcsecond of Declination (J2000) (4) 33- 37 F5.2 mag 3.6mag Spitzer 3.6µm band AB magnitude 39- 42 F4.2 mag e_3.6mag Uncertainty in 3.6mag 44- 48 F5.2 mag 4.5mag Spitzer 4.5µm band AB magnitude 50- 53 F4.2 mag e_4.5mag Uncertainty in 4.5mag 55- 59 F5.2 mag 5.8mag Spitzer 5.8µm band AB magnitude 61- 64 F4.2 mag e_5.8mag Uncertainty in 5.8mag 66- 70 F5.2 mag 8.0mag Spitzer 8.0µm band AB magnitude 72- 75 F4.2 mag e_8.0mag Uncertainty in 8.0mag 77 A1 --- l_24mag Limit flag on 24mag 78- 82 F5.2 mag 24mag Spitzer 24µm band AB magnitude 84- 87 F4.2 mag e_24mag ? Uncertainty in 24mag 89-105 A17 --- OID Other identification(s) (5)
Note (1): The following X-ray sources are in the area covered by the IRAC and MIPS images, but were not detected in the mid-infrared: Chandra IDs 10 (XMM ID 19), 13 (XMM ID 84), 30, 36, 45, 52 and XMM IDs 60, 64, 78, 81, 96, 121, 123. Note (2): Source catalog number given in Table 3 of Nandra et al. (2005MNRAS.360L..39N), referred to in this paper as cNNN. Source designation in NED or Simbad is [NLA2005] NNN. Note (3): Source number in Table 2 of Waskett et al. (2004MNRAS.350..785W), referred to in this paper as XNNN. Source designation in NED or Simbad is [WEG2004] 14h-NNN. Note (4): As measured on the IRAC images. Note (5): Lists are: 15V = Fomalont et al. (1991AJ....102.1258F); CUDSS = Webb et al. (2003ApJ...597..680W); Westphal = Steidel et al. (2003, Cat. J/ApJ/592/728).
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Francois Ochsenbein [CDS] 19-Mar-2007
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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