J/ApJ/660/167       Spitzer AGN candidates in CDFN           (Donley+, 2007)

Spitzer power-law active galactic nucleus candidates in the Chandra Deep Field-North. Donley J.L., Rieke G.H., Perez-Gonzalez P.G., Rigby J.R., Alonso-Herrero A. <Astrophys. J., 660, 167-190 (2007)> =2007ApJ...660..167D 2007ApJ...660..167D
ADC_Keywords: Active gal. nuclei ; X-ray sources ; Radio sources ; Millimetric/submm sources Keywords: galaxies: active - infrared: galaxies - X-rays: galaxies Abstract: We define a sample of 62 galaxies in the Chandra Deep Field-North whose Spitzer IRAC SEDs exhibit the characteristic power-law emission expected of luminous AGNs. We study the multi-wavelength properties of this sample and compare the AGNs selected in this way to those selected via other Spitzer color-color criteria. Only 55% of the power-law galaxies are detected in the X-ray catalog at exposures of >0.5Ms, although a search for faint emission results in the detection of 85% of the power-law galaxies at the ≥2.5sigma detection level. Most of the remaining galaxies are likely to host AGNs that are heavily obscured in the X-ray. Because the power-law selection requires the AGNs to be energetically dominant in the near- and mid-infrared, the power-law galaxies comprise a significant fraction of the Spitzer-detected AGN population at high luminosities and redshifts. The high 24um detection fraction also points to a luminous population. The power-law galaxies comprise a subset of color-selected AGN candidates. Description: Spitzer was used to obtain MIPS and IRAC MIR observations of the CDF-N, with 1400 and 500s exposures, respectively. We use these MIPS GTO images in place of the GOODS Spitzer data because the former cover the full CDF-N, whereas the latter cover a field approximately 2 times smaller. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 109 62 Power-law galaxy sample table5.dat 65 603 Templates -------------------------------------------------------------------------------- Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 15 34 57.2 +23 30 10 Arp 220 = IC 1127 17 23 21.9 -00 17 00 IRAS 17208-0014 = PMN J1723-0016 13 44 42.1 +55 53 11 Mrk 273 = UGC 8696 ---------------------------------------------------------- See also: J/AJ/122/2810 : Chandra Deep Field North Survey. V. (Brandt+, 2001) J/AJ/124/2351 : Chandra Deep Field North survey. XII (Bauer+, 2002) J/AJ/126/539 : The Chandra Deep Fields North and South (Alexander+, 2003) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [CDFN] 6- 10 I5 --- CDFN CDFN number, [DRP2007] NNNNN in Simbad 12- 13 I2 h RAh Right ascension (J2000) 15- 16 I2 min RAm Right ascension (J2000) 18- 22 F5.2 s RAs Right ascension (J2000) 24 A1 --- DE- Declination sign (J2000) 25- 26 I2 deg DEd Declination (J2000) 28- 29 I2 arcmin DEm Declination (J2000) 31- 35 F5.2 arcsec DEs Declination (J2000) 37- 40 F4.2 --- Pchi χ2 probability for power-law fit (see section 3 of paper) 42- 46 F5.2 --- alpha IRAC spectral index (f(ν)∝νalpha) 48- 51 F4.2 --- z ?=- Redshift 53- 56 F4.2 --- e_z ? rms uncertainty on z 58 A1 --- l_F24um Limit flag on F24um 59- 64 F6.1 uJy F24um ? 24um flux density 66 A1 --- l_F1.4G Limit flag on F1.4G 67- 72 F6.1 uJy F1.4G 1.4GHz flux density 74 A1 --- l_FX Limit flag on FX 75- 82 E8.3 mW/m2 FX 0.5-8keV X-ray flux 84 A1 --- l_logLX Limit flag on logLX 85- 88 F4.1 [10-7W] logLX ?=- X-ray luminosity in 0.5-8keV 90- 97 E8.3 s Exp X-ray exposure time 99-102 F4.1 arcmin theta X-ray off-axis angle 104 A1 --- l_q Limit flag on q 105-109 F5.2 [-] q ?=- Flux ratio, log(F24um/F1.4G) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 E10.4 um Arp.w The Arp 220 template wavelength 12- 21 E10.4 Jy Arp.F The Arp 220 template flux density 23- 32 E10.4 um IRAS.w ? The IRAS 17208-0014 template wavelength 34- 43 E10.4 Jy IRAS.F ? The IRAS 17208-0014 template flux density 45- 54 E10.4 um Mrk.w ? The Mrk 273 template wavelength 56- 65 E10.4 Jy Mrk.F ? The Mrk 273 template flux density -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 04-Mar-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