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J/ApJS/121/473 A diagnostic diagram for Seyfert 2 Galaxies (Bassani+, 1999)
A Three-dimensional Diagnostic Diagram for Seyfert 2 Galaxies: Probing X-Ray Absorption and Compton Thickness Bassani L., Dadina M., Maiolino R., Salvati M., Risaliti G., Della Ceca R., Matt G., Zamorani G. <Astrophys. J. Suppl. Ser. 121, 473 (1999)> =1999ApJS..121..473B (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, Seyfert; X-ray sources Keywords: galaxies: Seyfert - X-rays: galaxies Abstract: We present and discuss a three-dimensional diagnostic diagram for Seyfert 2 galaxies obtained using X-ray and [O III] data on a large sample of objects (reported in the Appendix). The diagram shows the Kα iron line equivalent width as a function of both the column density derived from the photoelectric cutoff and the 2-10 keV flux normalized to the [O III] optical-line flux (the latter corrected for extinction and assumed to be a true indicator of the source intrinsic luminosity). We find that the hard X-ray properties of type 2 objects depend on a single parameter, the absorbing column density along the line of sight, in accordance with the unified model. The diagram can be used to identify Compton-thick sources and to isolate and study peculiar objects. From this analysis we have obtained a column density distribution of Seyfert 2 galaxies that is thought to be a good approximation of the real distribution. A large population of heavily absorbed objects is discovered, including many Compton-thick candidates. Our results indicate that the mean log NHcm-2 in type 2 Seyfert galaxies is 23.5 and that as many as 23%-30% of sources have NH=>1024cm-2. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 130 73 Catalog of Seyfert 2 Galaxies table2.dat 131 73 Seyfert 2 spectral parameters refs.dat 140 98 References for table1.dat and table2.dat
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 19 A19 --- Name Seyfert galaxy name 21- 22 I2 h RAh Right Ascension (J2000) 24- 25 I2 min RAm Right Ascension (J2000) 27- 30 F4.1 s RAs Right Ascension (J2000) 33 A1 --- DE- Sign of the Declination (J2000) 34- 35 I2 deg DEd Declination (J2000) 37- 38 I2 arcmin DEm Declination (J2000) 40- 41 I2 arcsec DEs Declination (J2000) 43- 50 F8.5 --- z Redshift 52- 63 A12 --- Class Seyfert classification: S=Seyfert, L=Liner, SB=Starburst 64- 70 A7 --- r_z Reference for z and Class in refs.dat 72- 76 F5.2 10+20cm-2 ColD Galactic H I column density 82 A1 --- l_Rat Limit on Rat 83- 87 F5.2 --- Rat ? Ratio of Hα to H[beta 90- 99 A10 --- r_ColD References for ColD and Rat in refs.dat 101 A1 --- l_OIII Limit on OIII 102-107 F6.3 10-11mW/m2 OIII ? Corrected [O III] flux 109-113 F5.3 10-11mW/m2 e_OIII ? uncertainty on the [O III] flux 118 A1 --- n_OIII Remark on OIII (1) 121-130 A10 --- r_OIII References for OIII in refs.dat
Note (1): For this object, the only [O III] measurement available was taken with an aperture smaller than 100 pc as projected on the source, and therefore these data are likely to miss a significant fraction of the [O III] flux
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 19 A19 --- Name Seyfert Galaxy name 21 A1 --- n_Name [ehg] Name flag (1) 24- 28 F5.2 --- Gamma The photon index 30- 34 F5.2 --- E_Gamma ? upper limit on Gamma 36- 40 F5.2 --- e_Gamma ? lower limit on Gamma 42 A1 --- n_Gamma [fj] note on Gamma: f = Fixed photon index, j = Parameter is pegged at the higher limit 45 A1 --- l_ColD Lower limit on ColD 46- 52 F7.1 10+20cm-2 ColD Hydrogen column density 55 A1 --- n_ColD Flag indicating ColD and p_ColD is a range 58- 64 F7.1 10+20cm-2 E_ColD ? Upper limit on ColD 67- 74 F8.1 10+20cm-2 e_ColD ? Lower limit on ColD 76 A1 --- f_ColD [d] Indicates parameter is pegged at lower limit 78 A1 --- l_EW Lower limit on EW 79- 83 I5 eV EW ? Iron Kα line equivalent width 85- 90 I6 eV E_EW ? Upper limit on EW 93- 98 I6 eV e_EW ? Lower limit on EW 100 A1 --- n_EW Flag indicating line in EW is at 6.7 KeV 103-108 F6.4 10-11mW/m2 Fxo Observed flux between 2-10 KeV 112-118 F7.4 10-11mW/m2 Fxc Absorption corrected flux between 2-10 KeV 120 A1 --- n_Fxc Flag indicating Fxc is the lower value 124-127 F4.2 10-11mW/m2 E_Fxc ? Upper absorption corrected flux between 2-10 KeV 130-131 I2 --- r_Name References in refs.dat
Note (1): e = Compton-thick source with NH=>1025cm-2 g = Compton-thick source with NH=>1024cm-2 h = X-ray emission possibly dominated by a cooling flow around F09104+4109 (Fabian & Crawford, 1995MNRAS..274L..63F) and by intracluster emission in Cygnus A (Ueno+, 1994ApJ..431L..1U)
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Seq Sequence number from table1.dat 5- 23 A19 --- Bibcode Reference code sequence 26-140 A115 --- Com Comments on references
History: From ApJ electronic edition
(End) Greg Schwarz (AAS) 01-Feb-2000
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