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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).

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