Table 1.
Observational details of each sources.
| Source | AGN (a) | log flux (b) | Redshift | Instrument | Sequence | Start time | Exposure time | Net spectral counts (c) |
|---|---|---|---|---|---|---|---|---|
| Types | in erg cm−2 s−1 | (z) | ObsID | (UTC) | (ks) | |||
| XMM-Newton | 0762920601 | 2016-03-01 | 30.0 | 753, 225, 270 | ||||
| MCG-02-12-017 | Sy2 candidate | 8.84 | 0.03246 | NuSTAR | 60001160002 | 2014-11-28 | 34.0 | 441, 379 |
| NuSTAR | 60101015002 | 2016-03-02 | 19.5 | 349, 369 | ||||
| Chandra | 9438 | 2008-11-16 | 2.1 | 6 | ||||
| NGC 4180 | Sy2 | 17.58 | 0.00699 | NuSTAR | 60201038002 | 2016-07-14 | 23.4 | 429, 387 |
| NuSTAR | 60160480002 | 2020-07-14 | 31.6 | 212, 212 | ||||
| Swift-XRT | ( * ) | 2008—2020 | 17.8 (d) | 34 | ||||
| NGC 2788A | Sy2 | 21.46 | 0.01335 | NuSTAR | 60469001002 | 2019-06-14 | 27.6 | 608, 617 |
| NuSTAR | 60160344002 | 2020-08-14 | 23.2 | 639, 530 | ||||
| XMM-Newton | 0821870301 | 2019-03-02 | 32.6 | 1129, 257, 422 | ||||
| NGC 1106 | Sy2 | 15.49 | 0.01447 | NuSTAR | 60469002002 | 2019-02-22 | 18.7 | 285, 332 |
| NuSTAR | 60160130002 | 2020-09-09 | 22.3 | 360, 354 | ||||
| Chandra | 14050 | 2012-06-07 | 5.1 | 25 | ||||
| ESO406-G004 | Sy2 | 12.38 | 0.02897 | NuSTAR | 60201039002 | 2016-05-25 | 36.3 | 390, 357 |
| NuSTAR | 60161799002 | 2020-06-26 | 23.7 | 120, 86 | ||||
| XMM-Newton | 0802450501 | 2017-11-18 | 44.8 | 5232, 1980, 1134 | ||||
| 2MASX | Sy2 | 10.55 | 0.04422 | Chandra | 21299 | 2018-12-17 | 3.7 | 532 |
| J20145928+2523010 | NuSTAR | 60201032002 | 2017-05-27 | 28.1 | 1252, 1137 | |||
| NuSTAR | 60160731002 | 2020-04-21 | 9.4 | 608, 624 | ||||
| XMM-Newton | 0690580101 | 2013-02-24 | 135.4 | 27058, 8878, 9016 | ||||
| ESO138-G001 | Sy2 | 19.46 | 0.00914 | NuSTAR | 60201040002 | 2016-05-22 | 45.7 | 3101, 2806 |
| NuSTAR | 60061274002 | 2020-04-01 | 53.2 | 3463, 3328 | ||||
Notes.
AGN types and log flux between 14 and 195 keV is reported from the 105 month BAT catalogue of Oh et al. (2018). Only for ESO406-G004 is the AGN type reported from Koss et al. (2016).
The reported XMM-Newton net counts (background-subtracted total source counts) are those of the PN, MOS1, and MOS2 modules for a radius of 30″ in 0.3–10 keV, respectively. The reported NuSTAR net counts are those of the FPMA and FPMB modules for a radius of 30″ between 3 and 50 keV, respectively. The reported Chandra net counts are for the ACIS-I detector for a radius of 5″ in 0.5–7 keV. The reported Swift-XRT net counts are for a radius of 12″ in 0.5–10 keV.
( * )Collection of the following ObsID- 00081038001, 00037312004, 00037312001, 00037312002, 00037312003, 03106140005, 03106140004, 03106140001, 03106140002, 07002346001, 07002347001.
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