J/MNRAS/492/719    Chandra observations of 2106 radio-quiet QSOs (Timlin+, 2020)

The correlations between optical/UV broad lines and X-ray emission from a large sample of quasars. Timlin J., Brandt W.N., Ni Q., Luo B., Schneider D., Vivek M., Yi W. <Mon. Not. R. Astron. Soc. 492, 719 (2020)> =2020MNRAS.492..719T 2020MNRAS.492..719T (SIMBAD/NED BibCode)
ADC_Keywords: QSOs ; X-ray sources ; Photometry, SDSS ; Equivalent widths Keywords: galaxies: active - quasars: emission lines - quasars: general - X-rays: general Abstract: We present Chandra observations of 2106 radio-quiet quasars in the redshift range 1.7≤z≤2.7 from the Sloan Digital Sky Survey (SDSS), through data release fourteen (DR14, 2018ApJS..235...42A 2018ApJS..235...42A), that do not contain broad absorption lines (BAL) in their rest-frame UV spectra. This sample adds over a decade worth of SDSS and Chandra observations to our previously published sample of 139 quasars from SDSS DR5 which is still used to correlate X-ray and optical/UV emission in typical quasars. We fit the SDSS spectra for 753 of the quasars in our sample that have high-quality (large exposure time and small off-axis observation angle) X-ray observations, and analyze their X-ray properties (aox and daox) with respect to the measured CIV and MgII emission-line rest-frame equivalent width (EW) and the CIV emission-line blueshift. We find significant correlations (at the ≥99.99% level) between aox and these emission-line parameters, as well as between daox and CIV EW. Slight correlations are found between daox and CIV blueshift, MgII EW, and the ratio of CIV EW to MgII EW. The best-fit trend in each parameter space is used to compare the X-ray weakness (daox) and optical/UV emission properties of typical quasars and weak-line quasars (WLQs). The WLQs clearly deviate from the expectation for every relationship, typically exhibiting much weaker X-ray emission than predicted by the typical quasar relationships. The best-fit relationships for our typical quasars are consistent with predictions from the disk-wind quasar model. The behavior of the WLQs with respect to our typical quasars can be explained by an X-ray shielding model. Description: We assembled a large sample of 2106 quasars from the full SDSS quasar archive (through DR14) that were serendipitously observed with Chandra and are within the redshift range 1.7≤z≤2.7. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 1380 2106 Catalog catalog.fits 2880 558 fits version of the catalog -------------------------------------------------------------------------------- See also: http://skyserver.sdss.org/DR14 : SDSS DR14 Home Page Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 18 A18 --- SDSS SDSS Name (SDSS_Name) 20- 35 F16.12 deg RAdeg Right Ascension (J2000) (RA) 37- 54 F18.14 deg DEdeg [-10.6/69.7]? Declination (J2000) (DEC) 56- 68 F13.11 --- z [1.7/2.7]? Redshift (Z) 70- 82 F13.10 [cm-2] logNH [19.6/21.2]? Galactic column density (LOGNH) 84- 91 F8.4 mag IMAGZ2 [-30.0/-21.0]? Absolute Magnitude (corrected to z=2) (MI_Z2) 93- 99 A7 --- ObsID Chandra observation ID (ObsID) 101- 115 F15.12 arcmin Theta [0.1/19.4]? Chandra offaxis angle (THETA) 117- 132 F16.9 s ExpTimeS [737/170430]? Soft Band exposure time (ExposureTimesoft) 134- 149 F16.9 s ExpTimeH [737/170430]? Hard Band exposure time (ExposureTimehard) 151- 168 E18.12 --- PbSoft Binomial probability of detection (soft band) (Pb_soft) 170- 187 E18.12 --- PbHard Binomial probability of detection (hard band) (Pb_hard) 189- 204 F16.11 ct Soft-cts [1.9/1936.5]? Net soft-band counts (Soft_Cts) 206- 220 F15.11 ct E_Soft-cts [2.3/115.3]? Positive error (or upper limit) of net counts (soft band) (Softctsperr) 222- 238 F17.13 ct e_Soft-cts [0.0/107.9]? Negative error (or lower limit) of net counts (soft band) (Softctsmerr) 240- 254 F15.11 ct Hard-cts [2.0/674.4]? Net hard-band counts (Hard_cts) 256- 269 F14.11 ct E_Hard-cts [2.3/84.8]? Positive error (or upper limit) of net counts (hard band) (Hardctsperr) 271- 286 F16.13 ct e_Hard-cts [0.0/57.2]? Negative error (or lower limit) of net counts (hard band) (Hardctsmerr) 288- 303 F16.13 --- HR [0.0/29.8]? Hardness Ratio (HRat) 305- 321 F17.13 --- e_HR [0.0/784.5]? Negative error of hardness ratio (HR_merr) 323- 339 F17.14 --- E_HR [0.0/28.9]? Positive error of hardness ratio (HR_perr) 341- 343 F3.1 --- Gamma [0.5/3.0]? Power-law photon index (both band detections) or limit (single-band detection) (Gamma) 345- 348 F4.1 --- E_Gamma [-0.9/1.0]? Power-law photon index positive error (Gamma_perr) 350- 353 F4.1 --- e_Gamma [-0.4/0.6]? Power-law photon index negative error (Gamma) 355- 371 E17.12 ct/s Soft-Count-rate Soft-band count rate (SoftCountrate) 373- 389 E17.12 ct/s E_Soft-Count-rate Positive error on soft-band count rate (SoftCountrate_perr) 391- 407 E17.12 ct/s e_Soft-Count-rate Negative error on soft-band count rate (SoftCountrate_merr) 409- 418 E10.5 mW/m2 Soft-flux 0.5-2 keV flux (Soft_flux) 420- 429 E10.5 mW/m2 e_Soft-flux 0.5-2 keV flux lower limit (Softfluxlolim) 431- 440 E10.5 mW/m2 E_Soft-flux 0.5-2 keV flux upper limit (Softfluxuplim) 442- 458 E17.12 10-7J/cm2 F2kev Rest-frame 2 keV flux density (f2kev) 460- 476 E17.12 10-7J/cm2 bF2kev Rest-frame 2 keV flux density lower limit (f2kev_lolim) 478- 494 E17.12 10-7J/cm2 BF2kev Rest-frame 2 keV flux density upper limit (f2kev_uplim) 496- 508 F13.10 [10-7W] logL210kev [43.2/46.3]? Rest-frame 2-10 keV luminosity (logL_210kev) 510- 522 F13.10 [10-7W] blogL210kev [43.4/46.3]? Rest-frame 2-10 keV luminosity lower limit (logL210kevlolim) 524- 536 F13.10 [10-7W] BlogL210kev [42.8/46.2]? Rest-frame 2-10 keV luminosity upper limit (logL210kevuplim) 538- 554 E17.12 10-7J/cm2 F2500 Rest-frame 2500 Angstrom flux density (f2500) 556- 568 F13.10 [10-7W] logL2500 [28.9/32.2]? Rest-frame 2500Å luminosity density (logL_2500) 570- 584 F15.12 --- alphaox [-2.2/-0.4]? Observed alpha_ox (alphaox) 586- 600 F15.12 --- balphaox [-2.1/-0.5]? Observed alpha_ox lower limit (alphaox_lolim) 602- 616 F15.12 --- Balphaox [-2.4/-0.6]? Observed alpha_ox upper limit (alphaox_uplim) 618- 636 E19.12 --- dalphaox Difference between observed alpha_ox and the expectation from alpha_ox-L2500 relation (this work) (dalpha_ox) 638- 655 F18.15 --- dalphaoxJ07 [-0.5/0.8]? Difference between observed alpha_ox and the expectation from alpha_ox-L2500 relation (Just et al., 2007ApJ...665.1004J 2007ApJ...665.1004J) (dalphaoxJ07) 657- 675 E19.12 --- bdalphaox deltaalphaox lower limit (dalphaoxlolim) 677- 694 E18.12 --- Bdalphaox deltaalphaox upper limit (dalphaoxuplim) 696- 698 F3.1 --- ChipEdge [0/1]? If the Target overlapped with the edge of the Chandra CCD (1 for yes, 0 for no) (CHIP_EDGE) 700- 709 A10 "date" Obs.Date Date of the Chandra observation, iso-8601 (year) 711- 712 I2 --- ao [1.0/21.1]? Chandra observation cycle (ao) 714 I1 --- multobs [0/1]? Observed more than once in Chandra (1 for yes, 0 for no) (multobs) 716- 719 I4 --- Plate [269/8874]? SDSS spectroscopic Plate ID (PLATE) 721- 725 I5 --- MJD [51614/57520]? SDSS spectroscopic MJD (MJD) 727- 729 I3 --- Fiber [1/999]? SDSS spectroscopic Fiber ID (FIBER) 731- 743 F13.10 mag Umag0 [16.2/25.2]? Dereddend u-band apparent magnitude from SDSS (U_DERED) (1) 745- 757 F13.10 mag Gmag0 [16.0/23.0]? Dereddend g-band apparent magnitude from SDSS (G_DERED) (1) 759- 771 F13.10 mag Rmag0 [16.0/23.0]? Dereddend r-band apparent magnitude from SDSS (R_DERED) (1) 773- 785 F13.10 mag Imag0 [15.8/24.6]? Dereddend i-band apparent magnitude from SDSS (I_DERED) (1) 787- 799 F13.10 mag Zmag0 [15.6/23.5]? Dereddend z-band apparent magnitude from SDSS (Z_DERED) (1) 801- 803 I3 --- SDSSDR [71.0/142.1]? SDSS catalog in which the target was found (SDSS_DR) 805 I1 --- BALFlag [0/2]? Flag for detected broad absorption lines (BAL_FLAG) (2) 807- 808 I2 --- FIRSTFlag [-1/1]? Flag indicating if the source was detected in FIRST (FIRST_flag) (3) 810- 827 F18.15 mag Dg-i [-2.1/0.5]? SDSS g-i color relative to the mean (DELTAGI) 829 I1 --- FlagTexp-theta [0/1]? Flag which indicates if the target passed the exposure time -- offaxis angle cut (1= passed, 0=did not pass) (FlagTexptheta) 831- 846 F16.12 --- SNRcont [-1.0/41.9]? Measured signal-to-noise of the line free continuum regions (SNR_cont) 848- 861 F14.10 [107J/cm2] logf2500 [-29.3/-1.0]? logarithm of rest-frame 2500Å flux density measured from the spectrum (logf2500) 863- 878 F16.11 0.1nm CIV-EW [-1.0/857.2]? Rest-frame equivalent width of the CIV broad emission line measured directly from the spectrum (CIV_EW) 880- 896 F17.12 0.1nm e_CIV-EW [-1.0/160.3]? Measurement error of rest-frame equivalent width of the CIV broad emission line measured directly from the spectrum (CIVEWERR) 898- 913 F16.11 0.1nm CIV-EW-MOD [-1.0/960.4]? Rest-frame equivalent width of the CIV broad emission line measured from the Gaussian models (CIVEWMOD) 915- 931 F17.12 0.1nm e_CIV-EW-MOD [-1.0/165.8]? Measurement error of rest-frame equivalent width of the CIV broad emission line measured from the Gaussian models (CIVEWMOD_ERR) 933- 946 F14.8 km/s sigCIV-LINE [-1.0/5177.3]? Line dispersion of the CIV broad emission line (CIVLINESIGMA) 948- 961 F14.8 0.1nm CIV-peak [-1.0/1569.7]? Measured rest-frame peak of the CIV broad emission line (CIV_peak) 963- 978 F16.12 0.1nm e_CIV-peak [-1.0/15.6]? Uncertainty in the measured rest-frame peak of the CIV broad emission line (CIVpeakERR) 980- 994 F15.8 km/s CIV-FWHM [-1.0/22740.7]? Full Width Half Maximum of the modeled CIV broad emission line (CIV_FWHM) 996-1011 F16.9 km/s e_CIV-FWHM [-1.0/10596.8]? Uncertainty in Full Width Half Maximum of the modeled CIV broad emission line (CIVFWHMERR) 1013-1028 F16.12 --- CIV-LINE-SNR [-1.0/32.9]? Median Signal-to-Noise ratio of the CIV broad emission line (CIVLINESNR) 1030-1044 F15.10 0.1nm CIII-EW [-999.0/457.5]? Rest-frame equivalent width of the CIII broad emission line measured directly from the spectrum (CIII_EW) 1046-1062 F17.12 0.1nm e_CIII-EW [-999.0/231.1]? Measurement error of rest-frame equivalent width of the CIII broad emission line measured directly from the spectrum (CIIIEWERR) 1064-1078 F15.10 0.1nm CIII-EW-MOD [-999.0/310.3]? Rest-frame equivalent width of the CIII broad emission line measured from the Gaussian models (CIIIEWMOD) 1080-1096 F17.12 0.1nm e_CIII-EW-MOD [-999.0/193.8]? Measurement error of rest-frame equivalent width of the CIII broad emission line measured from the Gaussian models (CIIIEWMOD_ERR) 1098-1111 F14.8 km/s sigCIII-LINE [-999.0/6510.0]? Line dispersion of the CIII broad emission line (CIIILINESIGMA) 1113-1126 F14.8 0.1nm CIII-peak [-999.0/1937.7]? Measured rest-frame peak of the CIII broad emission line (CIII_peak) 1128-1144 F17.12 0.1nm e_CIII-peak [-999.0/20.0]? Uncertainty in the measured rest-frame peak of the CIII broad emission line (CIIIpeakERR) 1146-1160 F15.8 km/s CIII-FWHM [-999.0/37018.4]? Full Width Half Maximum of the modeled CIII broad emission line (CIII_FWHM) 1162-1176 F15.9 km/s e_CIII-FWHM [-999.0/8300.5]? Uncertainty in Full Width Half Maximum of the modeled CIII broad emission line (CIIIFWHMERR) 1178-1194 F17.12 --- CIII-LINE-SNR [-999.0/37.9]? Median Signal-to-Noise ratio of the CIII broad emission line (CIIILINESNR) 1196-1211 F16.10 0.1nm MgII-EW [-999.0/9357.6]? Rest-frame equivalent width of the MgII broad emission line measured directly from the spectrum (MgII_EW) 1213-1229 F17.12 0.1nm e_MgII-EW [-999.0/293.5]? Measurement error of rest-frame equivalent width of the MgII broad emission line measured directly from the spectrum (MgIIEWERR) 1231-1245 F15.10 0.1nm MgII-EWMOD [-999.0/617.3]? Rest-frame equivalent width of the MgII broad emission line measured from the Gaussian models (MgIIEWMOD) 1247-1263 F17.12 0.1nm e_MgII-EWMOD [-999.0/140.6]? Measurement error of rest-frame equivalent width of the MgII broad emission line measured from the Gaussian models (MgIIEWMOD_ERR) 1265-1278 F14.8 km/s sigMgII-LINE [-999.0/5950.5]? Line dispersion of the MgII broad emission line (MgIILINESIGMA) 1280-1293 F14.8 0.1nm MgII-peak [-999.0/2804.0]? Measured rest-frame peak of the MgII broad emission line (MgII_peak) 1295-1312 E18.12 0.1nm e_MgII-peak []?=-999 Uncertainty in the measured rest-frame peak of the MgII broad emission line (MgIIpeakERR) 1314-1328 F15.8 km/s MgII-FWHM [-999.0/35258.4]? Full Width Half Maximum of the modeled MgII broad emission line (MgII_FWHM) 1330-1345 F16.9 km/s e_MgII-FWHM [-999.0/11485.6]? Uncertainty in Full Width Half Maximum of the modeled MgII broad emission line (MgIIFWHMERR) 1347-1363 F17.12 --- MgII-LINE-SNR [-999.0/30.3]? Median Signal-to-Noise ratio of the MgII broad emission line (MgIILINESNR) 1365-1380 F16.12 --- RL [0.1/270.6]? Radio loudness parameter, F6cm/F2500Å (R6CM2500A) -------------------------------------------------------------------------------- Note (1): using Schlafly et al., 2011ApJ...737..103S 2011ApJ...737..103S. Note (2): Flag for detected broad absorption lines as follows: 0 = no line 1 = BAL 2 = mini-BAL Note (3): Flag indicating if the source was detected in FIRST as follows: -1 = target not covered by FIRST 0 = FIRST non-detection 1 = FIRST detected -------------------------------------------------------------------------------- Acknowledgements: John Timlin, jxt811(at)psu.edu
(End) Patricia Vannier [CDS] 03-Oct-2019
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