2005A&A...435..449J


C.D.S. - SIMBAD4 rel 1.7 - 2019.11.18CET18:54:50

2005A&A...435..449J - Astronomy and Astrophysics, volume 435, 449-457 (2005/5-4)

The XMM-Newton view of PG quasars. II. Properties of the Fe Kα line.

JIMENEZ-BAILON E., PICONCELLI E., GUAINAZZI M., SCHARTEL N., RODRIGUEZ-PASCUAL P.M. and SANTOS-LLEO M.

Abstract (from CDS):

The properties of the fluorescence Fe Kα emission lines of a sample of 38 quasars (QSOs) observed with XMM-Newton are studied. These objects are included in the optically selected sample from the Palomar-Green (PG) Bright Quasar Survey with an X-ray luminosity 1.3x1043<L2–10keV<5.1x1045erg/s and z≤1.72. For each object in the sample, we investigated the presence of both narrow and broad iron lines in detail. A total of 20 out of the 38 QSOs show evidence of an Fe Kα emission line with a narrow profile. The majority of the lines are consistent with an origin in low ionization material, which is likely to be located in the outer parts of the accretion disk, the molecular torus, and/or the Broad Line Region. The average properties of the narrow Fe Kα emission line observed in the sample are similar to those of Seyfert type galaxies as inferred from recent XMM-Newton and Chandra studies. A broad line has been significantly detected in only three objects. Furthermore, we studied the relationship between the equivalent width (EW) of the iron line and the hard band X-ray luminosity for radio quiet quasars. The analysis indicates that no clear correlation between the strength of the line and the hard X-ray luminosity is present, and our results do not show compelling evidence for an anticorrelation between these two quantities, i.e. the so-called X-ray Baldwin effect.

Abstract Copyright:

Journal keyword(s): galaxies: active - galaxies: nuclei - quasar: general - X-rays: galaxies

CDS comments: Table 1 PG 2303+029 is a probable misprint for PG 2302+029

Simbad objects: 45

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Number of rows : 45

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 Mrk 335 Sy1 00 06 19.5371542746 +20 12 10.617456059   14.19 13.85     ~ 1062 0
2 Mrk 1501 Sy1 00 10 31.0058529490 +10 58 29.505989476   15.96 15.40 12.22   ~ 625 0
3 Mrk 1502 Sy1 00 53 34.9326560879 +12 41 35.927159668   14.41 14.03     ~ 1008 1
4 Mrk 1014 Sy1 01 59 50.2529351498 +00 23 40.874250335   16.08 15.87     ~ 504 0
5 2MAXI J0808+757 Sy1 08 10 58.6637281539 +76 02 42.449416413   15.03 14.71     ~ 401 0
6 Ton 951 Sy1 08 47 42.4487014731 +34 45 04.483113429   14.83 14.50     ~ 404 0
7 2MASX J09504838+3926503 Sy1 09 50 48.3802745374 +39 26 50.463708894   16.83 16.73     ~ 166 0
8 PG 0953+414 Sy1 09 56 52.3930851607 +41 15 22.212153978 14.710 15.611 15.546 15.294 14.720 ~ 403 0
9 2MASS J10042013+0513004 Sy1 10 04 20.1377652635 +05 13 00.396937782   16.73 16.55     ~ 212 1
10 QSO B1048+342 Sy1 10 51 43.8919513785 +33 59 26.686941538   17.11 16.79     ~ 159 0
11 7C 110025.60+771511.00 Sy1 11 04 13.8613944317 +76 58 58.192391742   15.70 15.72 15.40   ~ 506 1
12 2MASSI J1117064+441333 Sy1 11 17 06.3986665282 +44 13 33.327898429   16.32 16.12     ~ 206 0
13 QSO B1115+080A QSO 11 18 16.951 +07 45 58.23   16.61 16.44     ~ 604 2
14 2MASSI J1118302+402553 Sy1 11 18 30.2896275867 +40 25 54.069567643   16.34 16.21     ~ 188 0
15 Ton 1388 Sy1 11 19 08.6786143504 +21 19 17.986556889   14.91 14.80     ~ 405 0
16 NGC 3783 Sy1 11 39 01.7095761008 -37 44 19.008597647   12.46 13.43 11.33 12.1 ~ 1446 0
17 2E 2584 Sy1 12 04 42.1097577213 +27 54 11.867990165   15.64 15.60     ~ 345 0
18 QSO J1208+4540 QSO 12 08 58.0106507296 +45 40 35.422302500   16.00 15.70     ~ 175 0
19 PB 3894 Sy1 12 14 17.6737003918 +14 03 13.182526431   14.46 14.19     ~ 723 0
20 PG 1216+069 Sy1 12 19 20.9316038223 +06 38 38.467864632   15.68 15.65     ~ 255 0
21 3C 273 BLL 12 29 06.6996828061 +02 03 08.598846466   13.05 14.830 14.11   ~ 5244 1
22 LBQS 1244+0238 Sy1 12 46 35.2527388863 +02 22 08.784237661   16.57 16.37     ~ 246 0
23 2E 2978 Sy1 13 09 47.0029670396 +08 19 48.215010428   16.04 15.89     ~ 333 0
24 Ton 1565 Sy1 13 12 17.7526648504 +35 15 21.087644341   15.45 15.64 14.2   ~ 236 1
25 2XMM J132349.6+654148 Sy1 13 23 49.5183330047 +65 41 48.166159616   16.01 15.84     ~ 152 0
26 ESO 383-35 Sy1 13 35 53.7686909139 -34 17 44.139127597   13.89 13.61 8.9   ~ 1361 0
27 PB 4142 Sy1 13 54 35.6873746503 +18 05 17.504062479   16.84 16.68     ~ 195 0
28 Ton 182 Sy1 14 05 16.2180155773 +25 55 34.116787862   15.42 15.34     ~ 226 0
29 2MASX J14062191+2223462 Sy1 14 06 21.8899286041 +22 23 46.515082049   16.62 16.42     ~ 200 0
30 QSO J1409+2618 QSO 14 09 23.9086975485 +26 18 21.053512073   16.07 15.74     ~ 179 0
31 2MASS J14134834+4400141 Sy1 14 13 48.3307115344 +44 00 14.005465999   14.99 14.99     ~ 339 0
32 2MASSI J1417008+445606 Sy1 14 17 00.8223053485 +44 56 06.331286859   16.93 16.63     ~ 219 0
33 NGC 5548 Sy1 14 17 59.5401093128 +25 08 12.600227883   14.35 13.73     ~ 2336 0
34 Mrk 1383 Sy1 14 29 06.5718492666 +01 17 06.155981953   15.21 14.87     ~ 396 0
35 2MASSI J1429430+474726 Sy1 14 29 43.0740635196 +47 47 26.215326061   17.29 16.97     ~ 152 0
36 Mrk 478 Sy1 14 42 07.4713423763 +35 26 22.939531895   14.91 14.58     ~ 476 0
37 2MASSI J1446459+403505 Sy1 14 46 45.9392876678 +40 35 05.797848407   16.28 16.11     ~ 259 0
38 Mrk 841 Sy1 15 04 01.1935077982 +10 26 15.778741853   14.50 14.27     ~ 574 0
39 7C 151247.00+370154.00 Sy1 15 14 43.0682940988 +36 50 50.355363752   17.11 17.01 15.83   ~ 374 1
40 Mrk 876 Sy1 16 13 57.1791807197 +65 43 09.953889666   16.03 15.49     ~ 497 0
41 QSO B1626+5529 Sy1 16 27 56.1124169072 +55 22 31.559608363   15.79 15.68     ~ 185 0
42 QSO B1630+3744 QSO 16 32 01.1118986024 +37 37 49.980862599   16.50 16.30     ~ 157 0
43 QSO B1634+7037 QSO 16 34 28.9917493918 +70 31 32.394595988   14.90 14.66     ~ 258 0
44 Mrk 304 Sy1 22 17 12.2638362727 +14 14 20.918554073   15.02 14.66     ~ 311 0
45 PB 5235 QSO 23 04 44.9533458555 +03 11 45.918742912   15.44 15.8     ~ 100 0

    Equat.    Gal    SGal    Ecl

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2019.11.18-18:54:50

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