J/A+A/645/A74       XMM-Newton spectral-fit redshift catalogue     (Ruiz+, 2021)

A search for X-ray absorbed sources in the 3XMM catalogue using photometric redshifts and Bayesian spectral fits. Ruiz A., Georgantopoulos I., Corral A. <Astron. Astrophys. 645, A74 (2021)> =2021A&A...645A..74R 2021A&A...645A..74R (SIMBAD/NED BibCode)
ADC_Keywords: X-ray sources ; Galaxies ; Active gal. nuclei ; Redshifts Keywords: catalogs - astronomical databases: miscellaneous - galaxies: active - X-rays: general - X-rays: galaxies Abstract: Since its launch in 1999, the XMM-Newton mission has compiled the largest catalogue of serendipitous X-ray sources, with the 3XMM being the third version of this catalogue. This is because of the combination of a large effective area (5000cm2 at 1keV) and a wide field of view (30 arcmin). The 3XMM-DR6 catalogue contains about 470000 unique X-ray sources over an area of 982deg2. A significant fraction of these (100178 sources) have reliable optical, near/mid-IR counterparts in the SDSS, PANSTARRS, VIDEO, UKIDSS and WISE surveys. In a previous paper we have presented photometric redshifts for these sources using the TPZ machine learning algorithm. About one fourth of these (22677) have adequate photon statistics so that a reliable X-ray spectrum can be extracted. Obviously, owing to both the X-ray counts selection and the optical counterpart constraint, the sample above is biased towards the bright sources. Here, we present XMMFITCAT-Z: a spectral fit catalogue for these sources using the Bayesian X-ray Analysis (BXA) technique. As a science demonstration of the potential of the present catalogue, we comment on the optical and mid-IR colours of the 765 X-ray absorbed sources with NH>1022cm-2. We show that a considerable fraction of X-ray selected AGN would not be classified as AGN following the mid-IR W1-W2 vs. W2 selection criterion. These are AGN with lower luminosities, where the contribution of the host galaxy to the MIR emission is non-negligible. Only one third of obscured AGN in X-rays present red colours or r-W2>6. Then it appears that the r-W2 criterion, often used in the literature for the selection of obscured AGN, produces very different X-ray absorbed AGN samples compared to the standard X-ray selection criteria. Description: The XMM-Newton spectral-fit Z catalogue (XMMFITCAT-Z) contains spectral- fitting results for 30816 detections, corresponding to 22,677 unique sources. This catalogue is produced by applying automated spectral fits to the EPIC spectral data contained within the XMM-Newton serendipitous source catalogue and using the distance information contained in XMMPZCAT. The version of the catalogue used to construct the current XMMFITCAT is 3XMM-DR6. 3XMM-DR6 is the third generation catalogue of serendipitous X-ray sources from the European Space Agency (ESA) XMM-Newton observatory, and has been created by the XMM-Newton Survey Science Centre (SSC) on behalf of ESA. The 3XMM-DR6 catalogue contains photometric information for 678,680 source detections, corresponding to 468,440 unique sources. As part of the catalogue production, spectra and time series are extracted in the case of detections with more than 100 counts collected in the EPIC camera. This corresponds to 149998 detections, and 102,157 unique sources. XMMPZCAT contains 100178 3XMM sources outside the Galactic plane (|b|>20deg) with highly reliable optical counterparts in the SDSS-DR13 or Pan-STARRS-DR1 catalogues. It offers photo-z for about 50% of the X-ray sources within the XMM-Newton observations selected for building the catalogue. The XMM-Newton spectral-fit database is constructed by using spectral data from the 3XMM-DR6 catalogue, but not all detections with extracted spectra are included in this database. To ensure the reliability of the spectral- fitting results, a constrain has been imposed to the number of counts collected in the X-ray spectra and as result, some detections are rejected in the automated spectral-fit pipeline. Moreover, only detections with redshifts in XMMPZCAT have been included. Here we also provide the sample of 977 X-ray absorbed AGN identified from the XMMFITCAT-Z catalogue, as presented in the paper. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file xfcz.dat 3198 30816 The XMM-Newton spectral-fit Z catalogue xfczabs.dat 529 977 Atlas of X-ray absorbed AGN -------------------------------------------------------------------------------- See also: IX/50 : XMM-Newton Serendipitous Source Catalogue 3XMM-DR6 (XMM-SSC, 2016) http://xraygroup.astro.noa.gr/Webpage-prodex/index.html : Enhanced XMM-Newton Spectral-fit Database Home Page Byte-by-byte Description of file: xfcz.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 20 A20 --- 3XMM IAU name assigned to the unique source in the 3XMM-DR6 catalogue (IAUNAME) 22- 41 F20.16 deg RAdeg Right ascension (J2000) of the unique source, as in the 3XMM-DR6 (SC_RA) (G1) 43- 62 E20.16 deg DEdeg Declination (J2000) of the unique source, as in the 3XMM-DR6 (SC_DEC) (G1) 64- 78 I15 --- Source Unique number assigned to a group of catalogue entries that are assumed to be the same source in 3XMM-DR6 (SRCID) 80- 94 I15 --- DetID Consecutive number that identifies each entry in the 3XMM-DR6 (DETID) 96- 105 I10 --- ObsID XMM-Newton observation identification, as in 3XMM-DR6 (OBS_ID) 107- 109 I3 --- SrcNum Source number (decimal) in the individual source list for this observation (OBS_ID), as in 3XMM-DR6 (SRC_NUM) 111- 116 F6.4 --- zphot Photometric redshift of the source from XMMPZCAT (PHOT_Z) 118- 123 F6.4 --- e_zphot Error of PHOT_Z from XMMPZCAT (PHOT_ZERR) 125- 143 E19.16 --- zsp ? Spectroscopic redshift of the source (SPEC_Z) 145- 165 E21.16 --- NHGAL Galactic hydrogen column density (NHGAL) (G2) 167- 189 F23.15 ct ctFull Spectral-background-subtracted counts in the full [0.5-10keV] band (T_COUNTS) (G3) 191- 215 F25.17 ct ctSoft Spectral-background-subtracted counts in the soft [0.5-2keV] band (S_COUNTS) (G3) 217- 243 F27.19 ct ctHard Spectral-background-subtracted counts in the hard [2-10keV] band (H_COUNTS) (G3) 245- 249 A5 --- AFIT True if an acceptable fit, i.e. KS p-value >0.01, has been found for at least one of the models applied, false otherwise (A_FIT) 251- 259 A9 --- Pmodel Data-preferred model, i.e. the model with lowest logZ (P_MODEL) 261- 284 A24 --- Amodels List of acceptable models (A_MODELS) (G4) 286- 306 F21.15 --- wapoWstat W-stat (Cash statistics) value for wapo model (wapo_wstat) (G5) 308- 314 F7.1 --- wapoDOF Degrees of freedom for wapo model (wapoDOF) 316- 336 F21.19 --- wapoKS Kolmogorov-Smirnov (KS) statistic for wapo model (wapo_ks) 338- 342 F5.3 --- wapoKSpvalue KS p-value for wapo model (wapokspvalue) 344- 365 F22.15 --- wapologZ Natural log of the evidence estimated by MultiNest for wapo model (wapo_logZ) 367- 384 F18.15 [cm-2] wapologNH Decimal log of the hydrogen column density for wapo model (wapologNH) 386- 403 F18.15 [cm-2] e_wapologNH Lower limit of the 90% credible interval for logNH for wapo model (wapologNH_min) 405- 422 F18.15 [cm-2] E_wapologNH Upper limit of the 90% credible interval for logNH for wapo model (wapologNH_max) 424- 441 F18.16 --- wapoPI Photon index for wapo model (wapoPI) 443- 460 F18.16 --- e_wapoPI Lower limit of the 90% credible interval for PhoIndex for wapo model (wapoPI_min) 462- 479 F18.16 --- E_wapoPI Upper limit of the 90% credible interval for PhoIndex for wapo model (wapoPI_max) 481- 501 F21.19 --- wapoz ? Redshift for wapo model (G6) (wapoz) 503- 523 F21.19 --- e_wapoz ? Lower limit of the 90% credible interval for z for wapo model (wapoz) 525- 545 F21.19 --- E_wapoz ? Upper limit of the 90% credible interval for z for wapo model (wapoz) 547- 568 E22.16 mW/m2 wapoFluxSoft Soft band flux for wapo model (wapoFluxSoft) 570- 591 E22.16 mW/m2 e_wapoFluxSoft Lower limit of the 90% credible interval for flux_soft for wapo model (wapoFluxSoft) 593- 614 E22.16 mW/m2 E_wapoFluxSoft Upper limit of the 90% credible interval for flux_soft for wapo model (wapoFluxSoft) 616- 637 E22.16 mW/m2 wapoFluxHard Hard band flux for wapo model (wapofluxhard) 639- 660 E22.16 mW/m2 e_wapoFluxHard Lower limit of the 90% credible interval for flux_hard for wapo model (wapofluxminhard) 662- 683 E22.16 mW/m2 E_wapoFluxHard Upper limit of the 90% credible interval for flux_hard for wapo model (wapofluxmaxhard) 685- 706 E22.16 mW/m2 wapoIFluxSoft Soft band, absorption corrected flux for wapo model (wapointfluxsoft) 708- 729 E22.16 mW/m2 e_wapoIFluxSoft Lower limit of the 90% credible interval for intflux_soft for wapo model (wapointfluxminsoft) 731- 752 E22.16 mW/m2 E_wapoIFluxSoft Upper limit of the 90% credible interval for intflux_soft for wapo model (wapointfluxmaxsoft) 754- 775 E22.16 mW/m2 wapoIFluxHard Hard band, absorption corrected flux for wapo model (wapointfluxhard) 777- 798 E22.16 mW/m2 e_wapoIFluxHard Lower limit of the 90% credible interval for intflux_hard for wapo model (wapointfluxminhard) 800- 821 E22.16 mW/m2 E_wapoIFluxHard Upper limit of the 90% credible interval for intflux_hard for wapo model (wapointfluxmaxhard) 823- 843 E21.16 10-7W wapoLSoft Soft band luminosity for wapo model (wapoluminsoft) 845- 865 E21.16 10-7W e_wapoLSoft Lower limit of the 90% credible interval for lumin_soft for wapo model (wapoluminminsoft) 867- 887 E21.16 10-7W E_wapoLSoft Upper limit of the 90% credible interval for lumin_soft for wapo model (wapoluminmaxsoft) 889- 909 E21.16 10-7W wapoLHard Hard band luminosity for wapo model (wapoluminhard) 911- 931 E21.16 10-7W e_wapoLHard Lower limit of the 90% credible interval for lumin_hard for wapo model (wapoluminminhard) 933- 953 E21.16 10-7W E_wapoLHard Upper limit of the 90% credible interval for lumin_hard for wapo model (wapoluminmaxhard) 955- 976 F22.15 --- wamekalWstat W-stat (Cash statistics) value for wamekal model (wamekal_wstat) (G5) 978- 984 F7.1 --- wamekalDOF Degrees of freedom for wamekal model (wamekal_dof) 986-1006 F21.19 --- wamekalKS Kolmogorov-Smirnov (KS) statistic for wamekal model (wamekal_ks) 1008-1012 F5.3 --- wamekalKSpvalue KS p-value for wamekal model (wamekalkspvalue) 1014-1036 F23.15 --- wamekallogZ Natural log of the evidence estimated by MultiNest for wamekal model (wamekal_logZ) 1038-1055 F18.15 [cm-2] wamekallogNH Decimal log of the hydrogen column density for wamekal (wamekal_logNH) 1057-1074 F18.15 [cm-2] e_wamekallogNH Lower limit of the 90% credible interval for logNH for wamekal model (wamekallogNHmin) 1076-1093 F18.15 [cm-2] E_wamekallogNH Upper limit of the 90% credible interval for logNH for wamekal model (wamekallogNHmax) 1095-1114 F20.17 --- wamekalkT Plasma temperature for wamekal model (wamekal_kT) 1116-1135 F20.17 --- e_wamekalkT Lower limit of the 90% credible interval for kT for wamekal model (wamekalkTmin) 1137-1156 F20.17 --- E_wamekalkT Upper limit of the 90% credible interval for kT for wamekal model (wamekalkTmax) 1158-1178 F21.19 --- wamekalz ? Redshift for wamekal model (wamekal_z) (G6) 1180-1200 F21.19 --- e_wamekalz ? Lower limit of the 90% credible interval for z for wamekal model (wamekalz_min) 1202-1222 F21.19 --- E_wamekalz ? Upper limit of the 90% credible interval for z for wamekal model (wamekalz_max) 1224-1245 E22.16 mW/m2 wamekalFluxSoft Soft band flux for wamekal model (wamekalfluxsoft) 1247-1268 E22.16 mW/m2 e_wamekalFluxSoft Lower limit of the 90% credible interval for flux_soft for wamekal model (wamekalfluxminsoft) 1270-1291 E22.16 mW/m2 E_wamekalFluxSoft Upper limit of the 90% credible interval for flux_soft for wamekal model (wamekalfluxmaxsoft) 1293-1314 E22.16 mW/m2 wamekalFluxHard Hard band flux for wamekal model (wamekalfluxhard) 1316-1337 E22.16 mW/m2 e_wamekalFluxHard Lower limit of the 90% credible interval for flux_hard for wamekal model (wamekalfluxminhard) 1339-1360 E22.16 mW/m2 E_wamekalFluxHard Upper limit of the 90% credible interval for flux_hard for wamekal model (wamekalfluxmaxhard) 1362-1383 E22.16 mW/m2 wamekalIFluxSoft Soft band, absorption corrected flux for wamekal model (wamekalintfluxsoft) 1385-1406 E22.16 mW/m2 e_wamekalIFluxSoft Lower limit of the 90% credible interval for intflux_soft for wamekal model (wamekalintfluxminsoft) 1408-1429 E22.16 mW/m2 E_wamekalIFluxSoft Upper limit of the 90% credible interval for intflux_soft for wamekal model (wamekalintfluxmaxsoft) 1431-1452 E22.16 mW/m2 wamekalIFluxHard Hard band, absorption corrected flux for wamekal model (wamekalintfluxhard) 1454-1475 E22.16 mW/m2 e_wamekalIFluxHard Lower limit of the 90% credible interval for intflux_hard for wamekal model (wamekalintfluxminhard) 1477-1498 E22.16 mW/m2 E_wamekalIFluxHard Upper limit of the 90% credible interval for intflux_hard for wamekal model (wamekalintfluxmaxhard) 1500-1520 E21.16 10-7W wamekalLSoft Soft band luminosity for wamekal model (wamekalluminsoft) 1522-1543 E22.17 10-7W e_wamekalLSoft Lower limit of the 90% credible interval for lumin_soft for wamekal model (wamekalluminminsoft) 1545-1565 E21.16 10-7W E_wamekalLSoft Upper limit of the 90% credible interval for lumin_soft for wamekal model (wamekalluminmaxsoft) 1567-1587 E21.16 10-7W wamekalLHard Hard band luminosity for wamekal model (wamekalluminhard) 1589-1609 E21.16 10-7W e_wamekalLHard Lower limit of the 90% credible interval for lumin_hard for wamekal model (wamekalluminminhard) 1611-1631 E21.16 10-7W E_wamekalLHard Upper limit of the 90% credible interval for lumin_hard for wamekal model (wamekalluminmaxhard) 1633-1652 F20.14 --- wamekalpoWstat ? W-stat (Cash statistics) value for wamekalpo (wamekalpo_wstat) (G5) 1654-1660 F7.1 --- wamekalpoDOF ? Degrees of freedom for wamekalpo model (wamekalpo_dof) 1662-1682 F21.19 --- wamekalpoKS ? Kolmogorov-Smirnov (KS) statistic for wamekalpo (wamekalpo_ks) 1684-1688 F5.3 --- wamekalpoKSpvalue ? KS p-value for wamekalpo (wamekalpokspvalue) 1690-1709 F20.14 --- wamekalpologZ ? Natural log of the evidence estimated by MultiNest for wamekalpo model (wamekalpo_logZ) 1711-1728 F18.15 [cm-2] wamekalpologNH1 ? Decimal log of the hydrogen column density for the outer component of wamekalpo (wamekalpo_logNH1) 1730-1747 F18.15 [cm-2] e_wamekalpologNH1 ? Lower limit of the 90% credible interval for logNH1 for wamekalpo model (wamekalpologNH1min) 1749-1766 F18.15 [cm-2] E_wamekalpologNH1 ? Upper limit of the 90% credible interval for logNH1 for wamekalpo model (wamekalpologNH1max) 1768-1785 F18.15 [cm-2] wamekalpologNH2 ? Decimal log of the hydrogen column density for the inner component of wamekalpo (wamekalpo_logNH2) 1787-1804 F18.15 [cm-2] e_wamekalpologNH2 ? Lower limit of the 90% credible interval for logNH2 for wamekalpo model (wamekalpologNH2min) 1806-1823 F18.15 [cm-2] E_wamekalpologNH2 ? Upper limit of the 90% credible interval for logNH2 for wamekalpo model (wamekalpologNH2max) 1825-1844 F20.17 --- wamekalpokT ? Plasma temperature for wamekalpo model (wamekalpo_kT) 1846-1865 F20.17 --- e_wamekalpokT ? Lower limit of the 90% credible interval for kT for wamekalpo model (wamekalpokTmin) 1867-1886 F20.17 --- E_wamekalpokT ? Upper limit of the 90% credible interval for kT for wamekalpo model (wamekalpokTmax) 1888-1905 F18.16 --- wamekalpoPI ? Photon index for wamekalpo (wamekalpo_PhoIndex) 1907-1924 F18.16 --- e_wamekalpoPI ? Lower limit of the 90% credible interval for PhoIndex for wamekalpo model (wamekalpoPhoIndexmin) 1926-1943 F18.16 --- E_wamekalpoPI ? Upper limit of the 90% credible interval for PhoIndex for wamekalpo model (wamekalpoPhoIndexmax) 1945-1965 F21.19 --- wamekalpoz ? Redshift for wamekalpo (wamekalpo_z) (G6) 1967-1987 F21.19 --- e_wamekalpoz ? Lower limit of the 90% credible interval for z for wamekalpo model (wamekalpoz_min) 1989-2009 F21.19 --- E_wamekalpoz ? Upper limit of the 90% credible interval for z for wamekalpo model (wamekalpoz_max) 2011-2032 E22.16 mW/m2 wamekalpoFluxSoft ? Soft band flux for wamekalpo model (wamekalpofluxsoft) 2034-2055 E22.16 mW/m2 e_wamekalpoFluxSoft ? Lower limit of the 90% credible interval for flux_soft for wamekalpo (wamekalpofluxminsoft) 2057-2078 E22.16 mW/m2 E_wamekalpoFluxSoft ? Upper limit of the 90% credible interval for flux_soft for wamekalpo (wamekalpofluxmaxsoft) 2080-2101 E22.16 mW/m2 wamekalpoFluxHard ? Hard band flux for wamekalpo model (wamekalpofluxhard) 2103-2124 E22.16 mW/m2 e_wamekalpoFluxHard ? Lower limit of the 90% credible interval for flux_hard for wamekalpo (wamekalpofluxminhard) 2126-2147 E22.16 mW/m2 E_wamekalpoFluxHard ? Upper limit of the 90% credible interval for flux_hard for wamekalpo (wamekalpofluxmaxhard) 2149-2170 E22.16 mW/m2 wamekalpoIFluxSoft ? Soft band, absorption corrected flux for wamekalpo model (wamekalpointfluxsoft) 2172-2193 E22.16 mW/m2 e_wamekalpoIFluxSoft ? Lower limit of the 90% credible interval for intflux_soft for wamekalpo (wamekalpointfluxminsoft) 2195-2216 E22.16 mW/m2 E_wamekalpoIFluxSoft ? Upper limit of the 90% credible interval for intflux_soft for wamekalpo (wamekalpointfluxmaxsoft) 2218-2239 E22.16 mW/m2 wamekalpoIFluxHard ? Hard band, absorption corrected flux for wamekalpo model (wamekalpointfluxhard) 2241-2262 E22.16 mW/m2 e_wamekalpoIFluxHard ? Upper limit of the 90% credible interval for intflux_hard for wamekalpo (wamekalpointfluxminhar) 2264-2285 E22.16 mW/m2 E_wamekalpoIFluxHard ? Lower limit of the 90% credible interval for intflux_hard for wamekalpo (wamekalpointfluxmaxhar) 2287-2307 E21.16 10-7W wamekalpoLSoft ? Soft band luminosity for wamekalpo model (wamekalpoluminsoft) 2309-2329 E21.16 10-7W e_wamekalpoLSoft ? Lower limit of the 90% credible interval for lumin_soft for wamekalpo (wamekalpoluminminsoft) 2331-2351 E21.16 10-7W E_wamekalpoLSoft ? Upper limit of the 90% credible interval for lumin_soft for wamekalpo (wamekalpoluminmaxsoft) 2353-2373 E21.16 10-7W wamekalpoLHard ? Hard band luminosity for wamekalpo model (wamekalpoluminhard) 2375-2395 E21.16 10-7W e_wamekalpoLHard ? Lower limit of the 90% credible interval for lumin_hard for wamekalpo (wamekalpoluminminhard) 2397-2417 E21.16 10-7W E_wamekalpoLHard ? Upper limit of the 90% credible interval for lumin_hard for wamekalpo (wamekalpoluminmaxhard) 2419-2438 F20.14 --- wapopoWstat ? W-stat (Cash statistics) value for wapopo (wapopo_wstat) (G5) 2440-2446 F7.1 --- wapopoDOF ? Degrees of freedom for wapopo model (wapopo_dof) 2448-2468 F21.19 --- wapopoKS ? Kolmogorov-Smirnov (KS) statistic for wapopo (wapopo_ks) 2470-2474 F5.3 --- wapopoKSpvalue ? KS p-value for wapopo (wapopokspvalue) 2476-2496 F21.14 --- wapopologZ ? Natural log of the evidence estimated by MultiNest for wapopo model (wapopo_logZ) 2498-2515 F18.15 [cm-2] wapopologNH1 ? Decimal log of the hydrogen column density for the outer component of wapopo (wapopo_logNH1) 2517-2534 F18.15 [cm-2] e_wapopologNH1 ? Lower limit of the 90% credible interval for logNH1 for wapopo model (wapopologNH1min) 2536-2553 F18.15 [cm-2] E_wapopologNH1 ? Upper limit of the 90% credible interval for logNH1 for wapopo model (wapopologNH1max) 2555-2572 F18.15 [cm-2] wapopologNH2 ? Decimal log of the hydrogen column density for the inner component of wapopo (wapopo_logNH2) 2574-2591 F18.15 [cm-2] e_wapopologNH2 ? Lower limit of the 90% credible interval for logNH2 for wapopo model (wapopologNH2min) 2593-2610 F18.15 [cm-2] E_wapopologNH2 ? Upper limit of the 90% credible interval for logNH2 for wapopo model (wapopologNH2max) 2612-2629 F18.16 --- wapopoPI1 ? Photon index for the outer component of wapopo (wapopo_PhoIndex1) 2631-2648 F18.16 --- e_wapopoPI1 ? Lower limit of the 90% credible interval for PhoIndex1 for wapopo model (wapopoPhoIndex1min) 2650-2667 F18.16 --- E_wapopoPI1 ? Upper limit of the 90% credible interval for PhoIndex1 for wapopo model (wapopoPhoIndex1max) 2669-2686 F18.16 --- wapopoPI2 ? Photon index for the inner component of wapopo (wapopo_PhoIndex2) 2688-2705 F18.16 --- e_wapopoPI2 ? Lower limit of the 90% credible interval for PhoIndex2 for wapopo model (wapopoPhoIndex2min) 2707-2724 F18.16 --- E_wapopoPI2 ? Upper limit of the 90% credible interval for PhoIndex2 for wapopo model (wapopoPhoIndex2max) 2726-2746 F21.19 --- wapopoz ? Redshift for wapopo (wapopo_z) (G6) 2748-2768 F21.19 --- e_wapopoz ? Lower limit of the 90% credible interval for z for wapopo model (wapopoz_min) 2770-2790 F21.19 --- E_wapopoz ? Upper limit of the 90% credible interval for z for wapopo model (wapopoz_max) 2792-2813 E22.16 mW/m2 wapopoFluxSoft ? Soft band flux for wapopo model (wapopofluxsoft) 2815-2836 E22.16 mW/m2 e_wapopoFluxSoft ? Lower limit of the 90% credible interval for flux_soft for wapopo (wapopofluxminsoft) 2838-2859 E22.16 mW/m2 E_wapopoFluxSoft ? Upper limit of the 90% credible interval for flux_soft for wapopo (wapopofluxmaxsoft) 2861-2882 E22.16 mW/m2 wapopoFluxHard ? Hard band flux for wapopo model (wapopofluxhard) 2884-2905 E22.16 mW/m2 e_wapopoFluxHard ? Lower limit of the 90% credible interval for flux_hard for wapopo (wapopofluxminhard) 2907-2928 E22.16 mW/m2 E_wapopoFluxHard ? Upper limit of the 90% credible interval for flux_hard for wapopo (wapopofluxmaxhard) 2930-2951 E22.16 mW/m2 wapopoIFluxSoft ? Soft band, absorption corrected flux for wapopo model (wapopointfluxsoft) 2953-2974 E22.16 mW/m2 e_wapopoIFluxSoft ? Lower limit of the 90% credible interval for intflux_soft for wapopo (wapopointfluxminsoft) 2976-2997 E22.16 mW/m2 E_wapopoIFluxSoft ? Upper limit of the 90% credible interval for intflux_soft for wapopo (wapopointfluxmaxsoft) 2999-3020 E22.16 mW/m2 wapopoIFluxHard ? Hard band, absorption corrected flux for wapopo model (wapopointfluxhard) 3022-3043 E22.16 mW/m2 e_wapopoIFluxHard ? Upper limit of the 90% credible interval for intflux_hard for wapopo (wapopointfluxminhard) 3045-3066 E22.16 mW/m2 E_wapopoIFluxHard ? Lower limit of the 90% credible interval for intflux_hard for wapopo (wapopointfluxmaxhard) 3068-3088 E21.16 10-7W wapopoLSoft ? Soft band luminosity for wapopo model (wapopoluminsoft) 3090-3110 E21.16 10-7W e_wapopoLSoft ? Lower limit of the 90% credible interval for lumin_soft for wapopo (wapopoluminminsoft) 3112-3132 E21.16 10-7W E_wapopoLSoft ? Upper limit of the 90% credible interval for lumin_soft (wapopoluminmaxsoft) 3134-3154 E21.16 10-7W wapopoLHard ? Hard band luminosity for wapopo model (wapopoluminhard) 3156-3176 E21.16 10-7W e_wapopoLHard ? Lower limit of the 90% credible interval for lumin_hard for wapopo (wapopoluminminhard) 3178-3198 E21.16 10-7W E_wapopoLHard ? Upper limit of the 90% credible interval for lumin_hard for wapopo (wapopoluminmaxhard) -------------------------------------------------------------------------------- Byte-by-byte Description of file: xfczabs.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 20 A20 --- 3XMM The IAU name assigned to the unique source in the 3XMM-DR6 catalogue (IAUNAME) 22- 39 F18.14 deg RAdeg Right ascension (J2000) of the unique source, as in the 3XMM-DR6 (SC_RA) (G1) 41- 60 F20.16 deg DEdeg Declination (J2000) of the unique source, as in the 3XMM-DR6 (SC_DEC) (G1) 62- 76 I15 --- Source Unique number assigned to a group of catalogue entries that are assumed to be the same source in 3XMM-DR6 (SRCID) 78- 92 I15 --- DetID Consecutive number that identifies each entry in the 3XMM-DR6 (DETID) 94-113 E20.15 cm-2 NHgal Galactic hydrogen column density (NHGAL) (G2) 115-136 F22.15 ct ctFull Spectral-background-subtracted counts in the full [0.5-10 keV] band (T_COUNTS) (G3) 138-161 F24.17 ct ctSoft Spectral-background-subtracted counts in the soft [0.5-2 keV] band (S_COUNTS) (G3) 163-184 F22.15 ct ctHard Spectral-background-subtracted counts in the hard [2-10 keV] band (H_COUNTS) (G3) 186-191 A6 --- Model Selected model for the spectral parameters (MODEL) (G6) 193-212 F20.18 --- z Redshift (z) 214-233 F20.18 --- E_z ? Upper error for z (z_ErrMax) 235-255 E21.19 --- e_z ? Lower error for z (z_ErrMin) 257-274 F18.15 [cm-2] logNH log10 of Hydrogen column density (logNH) (G7) 276-296 E21.19 [cm-2] E_logNH Upper error for logNH (logNH_ErrMax) 298-319 F22.19 [cm-2] e_logNH Lower error for logNH (logNH_ErrMin) 321-338 F18.16 --- PI Power law photon index (PhoIndex) (G7) 340-360 F21.19 --- E_PI Upper error for PhoIndex (PhoIndex_ErrMa) 362-382 E21.19 --- e_PI Lower error for PhoIndex (PhoIndex_ErrMi) 384-405 E22.16 mW/m2 FX Observed flux in total band (FX) 407-428 E22.16 mW/m2 E_FX Upper error for FX (FX_ErrMax) 430-451 E22.16 mW/m2 e_FX Lower error for FX (FX_ErrMin) 453-473 E21.16 [10-7W] LXHard Hard band X-ray luminosity (LX_HARD) 475-495 E21.16 [10-7W] E_LXHard Upper error for LX (LXHARDErrMax) 497-517 E21.16 [10-7W] e_LXHard Lower error for LX (LXHARDErrMin) 519-523 A5 --- highlogNH True if logNH > 22 (highNH) 525-529 A5 --- lowPI True if PhoIndex < 1.4 (lowPhoIndex) -------------------------------------------------------------------------------- Global notes: Note (G1): Corrected source coordinates and, in the case of multiple detections, they correspond to the weighted mean of the coordinates for the individual detections. Note (G2): Leiden/Argentine/Bonn (LAB) Survey of Galactic HI [Kalberla et al., 2005A&A...440..775K 2005A&A...440..775K, Cat. VIII/76] Note (G3): Computed by adding all available instruments and exposures for the corresponding observation Note (G4): This column contains the remaining models with relative evidence, with respect to P_MODEL, lower than 30, i.e. 'very strong evidence' accordingly to the scale of Jeffreys 1961. Assuming all models are a priori equally probable, there is no statistical reason to rule out any of the models in the set formed by P_MODEL and A_MODELS Note (G5): Models are: wapo = absorbed power law wamekal = absorbed thermal wamekalpo = absorbed thermal plus power law wapopo = absorbed double power law Note (G6): Null if spectroscopic redshift is available Note (G7): For the wapopo model, the spectral parameters corresponds to the inner component. -------------------------------------------------------------------------------- Acknowledgements: Angel Ruiz, ruizca(at)noa.gr This work is part of the Enhanced XMM-Newton Spectral-fit Database project, funded by the European Space Agency under the PRODEX program.
(End) Patricia Vannier [CDS] 18-Nov-2020
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