J/A+A/487/475  X-ray variability of AGNs in Lockman Hole   (Papadakis+, 2008)

The long-term X-ray variability properties of AGN in the Lockman Hole. Papadakis I.E., Chatzopoulos E., Athanasiadis D., Markowitz A., Georgantopoulos I. <Astron. Astrophys. 487, 475 (2008)> =2008A&A...487..475P 2008A&A...487..475P
ADC_Keywords: Active gal. nuclei ; X-ray sources ; Redshifts Keywords: galaxies: active - X-rays: galaxies Abstract: We present the results from a detailed X-ray variability analysis of 66 AGN in the Lockman Hole, which have optical spectroscopic identifications. We compare, quantitatively, their variability properties with the properties of local AGN, and we study the "variability - luminosity" relation as a function of redshift, and the "variability - redshift" relation in two luminosity bins. We use archival data from the last 10 XMM-Newton observations of the Lockman Hole field to extract light curves in the rest frame, 2-10keV band. We use the "normalized excess variance" to quantify the variability amplitude. Using the latest results regarding the AGN power spectral shape and its dependence on black hole mass and accretion rate, we are able to compute model "variability - luminosity" curves, which we compare with the relations we observe. When we consider all the sources in our sample, we find that their variability amplitude decreases with increasing redshift and luminosity. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 91 66 IDs, redshift, spectral and variability properties of AGN that we study in this work -------------------------------------------------------------------------------- See also: J/A+A/329/482 : ROSAT Deep Survey in the Lockman Hole (Hasinger+, 1998) J/PASJ/53/445 : ASCA Deep survey in Lockman Hole Field (Ishisaki+, 2001) J/A+A/393/425 : Spectral analysis of Lockman Hole (Mainieri+, 2002) J/A+A/398/901 : VLA survey at 6 cm in the Lockman Hole (Ciliegi+, 2003) J/A+A/413/843 : Far IR survey in the Lockman Hole (Kawara+, 2004) J/A+A/427/23 : 14.3um survey in the Lockman Hole (Fadda+, 2004) J/A+A/427/773 : ISOCAM 14.3um Deep Survey in Lockman Hole (Rodighiero+, 2004) J/AJ/128/1501 : CLASXS: X-ray catalog (Yang+, 2004) J/A+A/434/801 : X-ray sources near Lockman Hole (Zappacosta+, 2005) J/A+A/444/79 : XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005) J/A+A/473/105 : Lockman Hole AGN variability with XMM (Mateos+, 2007) J/A+A/479/283 : XMM observations of the Lockman Hole (Brunner+, 2008) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- [MBC2005] Source designation (1) 6- 7 I2 h RAh Right ascension (J2000) 9- 10 I2 min RAm Right ascension (J2000) 12- 16 F5.2 s RAs Right ascension (J2000) 18 A1 --- DE- Declination sign 19- 20 I2 deg DEd Declination (J2000) 22- 23 I2 arcmin DEm Declination (J2000) 25- 29 F5.2 arcsec DEs Declination (J2000) 31- 35 F5.3 --- z Redshift 37- 42 F6.3 --- snxs Normalized excess variance 44- 48 F5.3 --- e_snxs Error of snxs 50- 54 F5.2 --- logsnxs Logarithm of the snxs 56- 59 F4.2 --- e_logsnxs Error of the logarithm of snxs 61- 66 F6.1 --- chi2 Chi-square value 67 A1 --- --- [/] 68 I1 --- DOF Degrees of Freedom 70- 71 A2 --- Var [V NV] Variable/Non-Variable source flag 73- 77 F5.2 --- Lx Logarithm of luminosity in the [2-10]keV rest-frame band (1) 79- 82 F4.2 --- Gamma Power law spectral slope (1) 84- 91 A8 --- Inst Instrument(s) used in each case -------------------------------------------------------------------------------- Note (1): as in Table 8 of Mateos et al. (2005, Cat. J/A+A/444/79). -------------------------------------------------------------------------------- Acknowledgements: I.E. Papadakis, jhep(at)physics.uoc.gr
(End) Patricia Vannier [CDS] 29-May-2008
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