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Home All issues Volume 671 (March 2023) A&A, 671 (2023) A152 Full HTML
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Table A.1.

INTEGRAL/IBIS AGN

Name altern. name RA dec z class Log NH Γ2 − 10 keV F F Ref.
SWIFT J0001.6-7701 Fairall 1203 00 01 46.08 −76 57 14.3 0.058 Sy 1 22.69 1.8 (fixed) 3.39 0.72 1 (XRT)
NGC 235A - 00 42 52.81 −23 32 27.7 0.022 Sy 2 23.71 1.68 2.10 4.76 2
IGR J00569+6359 3PBC J0056.9+6401 00 57 12.70 +63 59 53.2 0.291 Sy 1.2 22.37 1.79 2.40 0.38 3
IGR J01036-6439 PKS 0101-649 01 03 33.74 −64 39 07.7 0.163 Blazar/QSO 20.41 1.66 3.00 1.12 3
IGR J01242+3348 NGC 513 01 24 26.80 +33 47 58.2 0.020 Sy 2 22.72 1.47 3.89 1.68 1 (XMM + NuSTAR)
SWIFT J0238.2-5213 ESO 198-24 02 38 19.72 −52 11 32.3 0.045 Sy 1 20.43 1.72 12.9 1.38 3
SWIFT J0250.2+4650 LEDA 2287192 02 50 27.18 +46 47 29.4 0.0210 Sy 2 22.38 1.36 6.40 1.63 1 (XRT)
IGR J03574-6602 NGC 1503 03 56 33.14 −66 02 27.6 0.019 AGN ∼23.26 1.8 (fixed) 0.34 0.75 1 (XRT)
SWIFT J0359.7+5058 4C 50.11 03 59 29.75 +50 57 50.2 1.520 Blazar/QSO 22.67 1.47 5.40 1.10 3
IGR J04059+5416 2MASX J04055765+5418446 04 05 57.66 +54 18 44.7 – AGN 22.54 1.50 1.10 1.08 4
IGR J04085-6546 LEDA 310383 04 08 38.82 −65 45 59.1 0.125 AGN 20.56 1.63 1.31 0.67 1 (XRT)
SWIFT J0414.8-0754 LEDA 14727 04 14 52.66 −07 55 39.7 0.038 Sy 1 20.73 1.97 5.00 1.79 3
NGC 1566 - 04 20 00.40 −54 56 16.6 0.005 Sy 1 19.93 1.73 3.10 2.20 3
SWIFT J0427.0+0734 2MASS J04270427+0716316 04 27 04.28 +07 16 31.7 0.096 Sy 1 20.94 1.61 4.20 0.83 1 (XRT)
IGR J04288-6702(1) LEDA 299570 04 29 47.48 −67 03 18.9 0.065 Sy 1.5 20.54 1.64 1.78 0.68 1 (XRT)
IGR J04426-0018(2) 1RXS J044229.8-001823 04 42 30.18 −00 18 29.1 0.449 Blazar/BL Lac 20.80 1.83 1.39 0.42 1 (XRT)
IGR J04426-0018(2) PKS 0440-003 04 42 38.59 −00 17 42.6 0.845 Blazar/QSO 20.80 1.92 1.32 0.42 1 (XRT)
IGR J05048-7340 ESO 33-11 05 05 06.27 −73 39 04.6 0.014 XBONG 20.15 1.8 0.33 0.47 1 (XRT)
IGR J05162-1034 MCG-02-14-009 05 16 21.22 −10 33 41.4 0.029 Sy 1 20.97 2.23 4.20 1.08 3
IGR J05511-1218 LEDA 148076 05 51 13.12 −12 14 42.1 0.035 XBONG 22.93 1.8 (fixed) 0.8 < 1.75 1 (XRT), 5, 6
SWIFT J0600.7+0008 IRAS05581+0006 06 00 40.11 +00 06 18.4 0.115 Sy 1.9 23.30 1.8 (fixed) 1.99 0.83 1 XRT
IGR J06075-6148 ESO 121-6 06 07 29.85 −61 48 27.3 0.004 AGN 23.33 1.89 0.95 0.73 7
IGR J06380-7536 LEDA 243576 06 37 43.17 −75 38 46.3 0.089 Sy 1.8 – – – 0.78 no (2-10) data
IGR J06503-7742⋆ LEDA 235040 06 49 54.37 −77 42 18.6 0.037 AGN – – 0.64 0.94 8
IGR J07072-1227 2MASX J07071126-1227560 07 07 11.43 −12 28 00.2 0.071 Sy 2 22.71 1.8 (fixed) 1.11 1.13 1 (XRT), 5
SWIFT J0710.5+5908 RX J0710.5+5908 07 10 30.07 +59 08 20.3 0.125 Blazar/BL Lac 20.65 1.80 28.5⋄ 2.28 1 (XRT)
IGR J07328-4640 PKS 0731-465 07 32 44.31 −46 40 17.2 – Blazar/QSO 21.18 1.8 (fixed) 1.99 0.89 1 (XRT)
RX J0818.9-2252 LEDA 80921 08 18 57.72 −22 52 36.2 0.035 Sy 1 21.05 1.79 3.46 0.93 1 (XRT)
SWIFT J0823.4-0457 Fairall 272 08 23 01.10 −04 56 05.4 0.022 Sy 2 23.23 1.51 6.46 2.22 9
IGR J08297-4250 2MASX J08294112-4251582 08 29 41.12 −42 51 58.3 – AGN 23.78 1.50 1.10 0.67 4
SWIFT J0835.5-0902(3) 2MASX J08353333-0905302 08 35 33.34 −09 05 30.2 0.112♣ AGN 20.62 2.04 1.68 1.62 1 (XRT)
NGC 2617 - 08 35 38.00 −04 05 17.9 0.014 Sy 1/1.8 23.34 1.87 23.5 5.00 10
PKS 0921-213 - 09 23 38.88 −21 35 47.1 0.053 Sy 1 20.63 1.77 6.23 1.60 1 (XRT)
SWIFT J0924.2-3142 2MASS J09235373-3141308 09 23 53.61 −31 41 31.6 0.042 Sy 1.8 23.91 1.8 (fixed) 1.7 2.26 11
SWIFT J0958.2-5732 WISEA J095834.97-572927.2 09 58 35.03 −57 29 26.7 – AGN 22.28 1.8 (fixed) 3.44 0.52 1
ESO 317-41 SWIFTJ1031.5-4205 10 31 23.11 −42 31 23.1 0.019* Sey 2 23.90 1.76 0.44 1.11 9
IGR J10447-6027 2MASS J10445192-6025115 10 44 51.91 −60 25 11.9 0.047 Sy 2 23.22 1.50 2.20 0.95 12
IGR J10595-5125 ESO 215-14 10 59 19.03 −51 26 32.3 0.019 Sy 1 21.10 1.65 5.71 0.55 1 (XRT)
IGR J11275-5319 2MASX J11273392-5320270 11 27 33.90 −53 20 25.9 0.049♣ AGN 23.18 1.8 (fixed) 0.84 0.97 1 (XRT)
IGR J11299-6557 2MASS J11295643-6555218 11 29 56.90 −65 55 18.9 – AGN < 22.04 2.09 3.20 0.53 1 (XRT)
RX J1136.5+6737 SWIFT J1136.7+6738 11 36 30.10 +67 37 04.0 0.134 Blazar/BL Lac 20.74 2.04 11.6 0.81 3
NGC 4102 - 12 06 23.11 +52 42 39.4 0.003 LINER 23.87 1.74 1.44 2.53 9
IGR J12418+78054, ⋆ LEDA 140000 12 42 36.10 +78 07 20.4 0.022 Sy 1.9 – – 1.00 0.94 8
PKS 1252+11 - 12 54 38.25 +11 41 05.9 0.872 Blazar/QSO 20.38 1.30 1.77 0.58 1 (XRT)
IGR J13045-5630 WISE J130431.77-563058.5 13 04 31.50 −56 30 54.8 – AGN 23.29 1.8 (fixed) 1.82 0.91 13
RX J1317.0+3735 - 13 17 02.89 +37 35 32.7 0.195 NLS1 – – 1.02 no (2-10) keV data
ESO 509-G038 - 13 31 13.84 −25 24 09.9 0.026 Sy 1 20.44 1.56 3.44 1.69 1 (XRT)
PKS 1413-36 - 14 16 33.16 −36 40 53.8 0.075 AGN 22.53 1.8 (fixed) 1.77 0.74 1 (XRT)
MRK 1383 - 14 29 06.57 +01 17 06.1 0.087 Sy 1 20.41 1.87 6.50 1.11 1 (XMM+NuSTAR)
MRK 817 - 14 36 22.08 +58 47 39.4 0.031 Sy 1.2 22.84 1.91 6.67 1.74 14
MRK 477 - 14 40 38.09 +53 30 16.2 0.038 Sy 2 23.30 1.58 3.38 1.27 9
IGR J14417-5533 WISE J144118.74-553335.1 14 41 18.94 −55 33 33.5 – AGN 21.57 1.55 7.38 0.89 1 (XRT)
IGR J14557-5448 LEDA 415943 14 55 32.19 −54 46 31.3 – AGN 23.15 1.8 (fixed) 0.44 0.58 1 (XMM)
IGR J16005-4645 PMN J1600-4649 16 00 20.40 −46 48 41.3 – AGN 22.08 1.8 (fixed) 4.40 0.46 1 (XRT)
3C 332.0 - 16 17 42.54 +32 22 34.4 0.151 Sy 1 22.01 1.77 9.22 1.12 1 (XRT + NuSTAR)
IGR J16181-5407 2MASS J16180771-5406122 16 18 07.74 −54 06 12.2 0.085 AGN 22.95 0.8 1.27 0.57 15
IGR J16246-4556 2MASS J16243080-4555144 16 24 30.77 −45 55 14.1 – AGN 22.40 1.3 0.93 < 0.59 15
IGR J16413-4046 CXOU J164119.4–404737 16 41 19.5 −40 47 37.7 – AGN 23 1.8 (fixed) 1.40 1.45 16
IGR J16459-2325 ESO 518-2 16 45 54.95 −23 27 05.5 0.020 AGN ∼23.78 1.8 (fixed) 4.30 1.58 1 (XRT)
IGR J16560-4958 CXOU J165551.9–495732 16 55 51.95 −49 57 32.4 – AGN 22.36 2.3 17.00 1.20 17
IGR J17157-5449 2MASS J17153752-5450062 17 15 37.53 −54 50 05.1 – AGN 21.12 1.51 4.25 0.59 1 (XRT)
IGR J17255-4509 2MASX J17253053-4510279 17 25 30.55 −45 10 27.3 0.019 AGN 21.25 1.8 (fixed) 2.91 0.54 1 (XRT)
SWIFT J1745.4+2906 1RXSJ174538.1+290823 17 45 38.29 +29 08 22.7 0.111 Sy 1 < 20.30 1.57 7.08 1.25 1 (XRT+ NuSTAR)
IGR J18134-1636 - 18 13 28.03 −16 35 48.5 – AGN 22.65 1.8 (fixed) 1.15 0.94 1 (XRT)
IGR J18141-1823 4PBC J1814.1-1822 18 14 14.78 −18 23 09.6 – AGN 22.68 1.8 (fixed) 0.98 0.63 1 (XRT)
AX J1830.6-1002 - 18 30 38.3 −10 02 47.1 – AGN 23.03 1.01 3.20 1.00 18
IGR J18381-0924 CXOU J183818.5-092552 18 38 18.58 −09 25 52.2 0.031 Sy 1.9 22.34 1.19 2.30 0.81 19
SWIFT J1839.1-5717 allWISE J183905.95-571505.1 18 39 06.37 −57 15 05.8 – AGN 22.31 1.57 8.40 1.27 11
IGR J18486-0047 CXOU J184825.4?004635 18 48 25.45 −00 46 34.9 – AGN 23.45 1.8 (fixed) 1.63 0.85 1 (XRT)
IGR J18497-0248 NVSS J184946-024819 18 49 46.67 −02 48 17.3 – AGN ∼22.60 1.8 (fixed) 1.08 0.70 1 (XRT)
IGR J19294+1328 CXOU J192930.1+132705 19 29 30.11 +13 27 05.6 – AGN 23.89 1.8 (fixed) 1.87 0.85 1(XRT), 14
SWIFT J1937.5-40212 LEDA 588288 19 37 13.47 −40 16 14.8 0.075 AGN 22.23 1.51 3.92 0.31 1(XRT)
SWIFT J1937.5-40212 1RXS J193716.1-401026 19 37 14.70 −40 10 14.9 – AGN 22.91 1.92 0.78 0.31 1(XRT)
IGR J19504+3319 2MASS J19501973+3314166 19 50 19.73 +33 14 16.2 – AGN 22.04 1.8 2.24 1.34 20
IGR J19577+3339 CXOU J195740.5+333828 19 57 40.59 +33 38 28.2 – AGN < 23.5 -0.6 0.26 0.53 20
IC 5063 - 20 52 02.33 −57 04 07.6 0.011 Sy 2 23.36 1.77 8.70 4.92 9
SWIFT J2055.0+3559 2MASS J20550835+3556278 20 55 08.23 +35 56 27.4 0.115♣ AGN 23.02 1.8 (fixed) 2.50 0.47 1 (XRT)
IGR J20569+4940 4C 49.35 20 56 42.74 +49 40 06.6 0.100♣ Blazar/BL Lac 22.54 2.60 22.0 1.16 12
IGR J20596+4303(5) - 21 00 01.00 +43 02 11.0 0.066 Sy 2 22.41 1.8 1.49 0.57 21
IGR J22018+5049 NRAO 676 22 01 43.54 +50 48 56.4 1.899 Blazar/QSO 21.57 1.39 5.20 0.99 1 (XRT)
AX J2254.3+1146(2) UGC 12237 22 54 19.67 +11 46 56.8 0.0286 Sy 2 23.06 1.8 (fixed) 3.10 0.51 1 (XRT)
AX J2254.7+1146(2) UGC 12243 22 54 43.51 +11 42 50.9 0.0278 Sy 1 20.71 1.75 0.13 0.51 1 (XRT)
1ES 2344+514 - 23 47 04.84 +51 42 17.9 0.044 Blazar/BL Lac 21.18 1.96 17.0 0.58 1 (XRT)

Notes: Sources in bold are (also) in cat 1000. Values of Log NH in bold are for sources where only Galactic absorption was measured; for the rest of the sample sources, the Galactic absorption was always considered in addition to the intrinsic one listed; ( † ) 2-10 keV flux in units of 10−12 erg cm−2 s−1; ( ‡ ) 20-100 keV flux in units of 10−11 erg cm−2 s−1. (1) Two sources are present within the IBIS error circle: a Seyfert 1 galaxy, whose values are reported in the table, and an eclipsing X-ray binary, a transitional millisecond pulsar (SXPS J042749.2-670434). Both sources were detected above 3 keV; therefore, the hard X-ray emission could be due to the contribution of the two sources. (2) Two sources are present within the IBIS error circle, both AGN, and both are reported in the table. The hard X-ray emission could be the result of the contribution of two objects, and therefore the value reported in Krivonos has been divided by two. (3) Two sources lie within the IBIS error circle: the galaxy 2MASX J08353333-0905302, with the photometric redshift reported in the table, and a rotationally variable star, ASAS J083531-0904.1. Both objects emit above 5 keV; therefore, they could both contribute to the hard X-ray emission. ( ⋆ ) For these sources, only the XMM Slew Survey flux is available. (4⋆) Two sources are listed in the XMM Slew Survey: LEDA140000 (also ROSAT Bright), reported in the table, and XMMSL2 J124313.8+780828, which is unidentified and has a 2-10 keV flux of 5.9 × 10−12 erg cm−2 s−1. Both sources probably contribute to the high-energy emission. (5) Two sources lie within the IBIS error circle. One is the Seyfert 2 reported in the table, while the second is a CV. They both contribute to the high-energy flux. ⋄ Mean value. ♣ Photometric redshift. * Redshift and optical class from Oh et al. (2022).

References: 1): This work; 2): Yamada et al. (2021); 3): Ricci et al. (2017); 4): Tomsick et al. (2015); 7): Annuar et al. (2020); 8) Saxton et al. (2008); 9) Zhao et al. (2021); 10) Giustini et al. (2017); 11) Landi et al. (2017); 12) Clavel et al. (2019); 13) Rodriguez et al. (2010); 14) Kara et al. (2021); 15) Tomsick et al. (2020); 16) Landi et al. (2011); 17) Tomsick et al. (2012) 18) Bassani et al. (2009); 19) Rahoui et al. (2017); 20) Tomsick et al. (2021) 21) Karasev et al. (2020)

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