Free Access

Table 1

2XMM-IRAS sample.

IRAS name 2XMM name IRAS-XMM ID Redshift XMM-optical Satellite X-ray class.
offset (′′) offset (′′)

00085 − 1223 J001106.5–120626 2.73 NGC 17 0.0196 0.06 XMM C-thick
00387 + 2513 J004128.0+252958 11.00 NGC 214∗∗ 0.0151 0.90 XMM+BAT C-thick
01091 − 3820 J011127.5–380500 3.00 NGC 424 0.0118 0.78 XMM+BAT C-thick
01306 + 3524 J013331.1+354006 2.80 NGC 591 0.0152 1.20 XMM C-thick
01413 + 0205 J014357.7+022059 10.80 Mrk 573 0.0172 1.08 XMM C-thick
02401 − 0013 J024240.7–000046 2.63 NGC 1068 0.0038 1.80 XMM+BAT C-thick
03012 − 0117 J030349.0–010613 2.60 NGC 1194 0.0136 0.66 XMM+BAT C-thick
03106 − 0254 J031308.7–024319 14.30 2MFGC 2636∗∗ 0.0272 0.18 XMM C-thick
03222 − 0313 iJ032448.6-030231 1.30 NGC 1320 0.0089 0.24 XMM+BAT C-thick
03317 − 3618 J033336.3–360825 5.80 NGC 1365 0.0055 0.18 XMM+BAT C-thick
03348 − 3609 J033646.1–355957 1.63 NGC 1386 0.0029 0.72 XMM C-thick
04507 + 0358 J045325.7+040342 5.30 CGCG 420-015∗∗ 0.0294 1.20 XMM+BAT+Suz. C-thick
05093 − 3427 J051109.0–342335 3.80 ESO 362-8∗∗ 0.0157 1.56 XMM C-thick
05189 − 2524 J052101.4–252144 3.89 IRAS 05189-2524 0.0426 0.43 XMM+BAT C-thin
06097 + 7103 J061536.2+710214 4.70 Mrk 3 0.0135 0.60 XMM+BAT C-thick
06456 + 6054 J065008.6+605044 2.60 NGC 2273 0.0061 0.18 XMM C-thick
07379 + 6517 iJ074241.6+651037 2.00 Mrk 78∗∗ 0.0372 0.42 XMM+BAT C-thick?5
08043 + 3908 J080741.0+390015 10.90 Mrk 622 0.0232 0.24 XMM C-thick?6
09320 + 6134 J093551.5+612111 0.90 UGC 05101 0.0394 0.66 XMM C-thick
09497 − 0122 J095219.1–013643 3.70 Mrk 1239 0.0199 0.72 XMM C-thin
09585 + 5555 J100157.8+554047 1.20 NGC 3079 0.0037 0.60 XMM+BAT C-thick
11538 + 5524 J115628.2+550732 6.40 NGC 3982 0.0037 2.34 XMM C-thick
12540 + 5708 J125614.2+565224 3.20 Mrk 231 0.0422 0.72 XMM C-thick
12550 − 2929 J125744.9–294558 10.17 ESO 443-17 0.0102 0.78 XMM C-thin
13044 − 2324 J130705.9–234036 1.30 NGC 4968 0.0099 1.20 XMM C-thick
13277 + 4727 J132952.5+471144 15.0 M51 0.0020 4.40 XMM C-thick
13362 + 4831 J133817.5+481637 7.14 Mrk 266 0.0279 3.88 XMM C-thick
13428 + 5608 J134442.1+555312 1.00 Mrk 273 0.0378 0.24 XMM+BAT C-thick
13536 + 1836 J135602.7+182218 1.20 Mrk 463 0.0503 1.80 XMM+BAT C-thin
15084 + 5711 J150947.0+570002 9.50 NGC 5879 0.0026 2.76 XMM (Low stat.)+Chandra C-thin
15295 + 2414 J153143.4+240420 14.00 3C 321 0.0961 1.50 XMM C-thick
15327 + 2340 J153457.3+233011 9.70 Arp220 0.0181 2.49 XMM C-thick?
15480 − 0344 J155041.6-035318 8.60 2MASXJ15504152-0353175 0.0303 1.68 XMM C-thick
16504 + 0228 J165258.9+022403 3.70 NGC 6240 0.0245 0.24 XMM+BAT C-thick
18429 − 6312 iJ184744.1–630924 6.50 IC 4769∗∗ 0.0151 0.66 XMM C-thick
19254 − 7245 J193121.5–723920 4.90 AM 1925-724 0.0617 2.52 XMM C-thick
20162 − 5246 J201958.9-523718 2.00 IC 4995 0.0161 1.02 XMM C-thin7
20305 − 0211 J203306.1-020128 6.50 NGC 6926 0.0196 10.08 XMM C-thick
22045 + 0959 J220702.0+101401 11.00 NGC 7212 0.0267 1.02 XMM+BAT C-thick?8
22469 − 1932 J224937.0-191627 7.00 MCG-03-58-007 0.0315 1.20 XMM+Suz. C-thin
23024 + 1203 J230456.6+121921 2.60 NGC 7479∗∗ 0.0079 0.90 XMM+BAT C-thick
23156 − 4238 J231823.5-422213 3.84 NGC 7582 0.0053 0.66 XMM+BAT C-thick
23254 + 0830 J232756.7+084645 3.50 NGC 7674 0.0289 0.72 XMM C-thick

Notes. Column 1: IRAS name; Col. 2: 2XMM name; Col. 3: offset in arcsec between the IRAS and the X-ray position; Col. 4: NED/SIMBAD name; Col. 5: redshift (from NED/SIMBAD); Col. 6: offset in arcsec between the XMM and the optical position; Col. 7: name of the satellite/instrument from which we have taken the X-ray data; Col. 8: X-ray classification. We mark with ∗∗ the seven newly discovered Compton-thick AGN.

(5)

This source is classified as Compton-thick AGN by using disk-reflection models and as Compton-thin by using the toroidal model (in agreement also with the analysis presented in Gilli et al. 2010).

(6)

This source is classified as Compton-thin AGN by using toroidal models and as Compton-thick by using the disk–reflection model (in agreement with the result of the analysis presented in Guainazzi et al. 2005).

(7)

This source was previously classified as Compton-thick by Guainazzi et al. (2005) and as Compton-thin by Noguchi et al. (2009).

(8)

This source is classified as Compton-thin AGN by using toroidal models and as Compton-thick by using the disk-reflection model (in agreement with the Della Ceca et al. 2008a, and references therein).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.