Table 2.
Main properties and statistics of the observations of Mrk 1018.
| Telescope | Date | ObsID | Exposure | Bkg level | Flux 0.5−2 keV | Flux 2−10 keV |
|---|---|---|---|---|---|---|
| [ks] | [10−12
 ] |
[10−12
 ] |
||||
| XMM-Newton | 15/01/2005 | 0201090201 | 1.61 | 4% | 6.47 |
9.52 |
| Swift-XRT | 29/06/2007 (a) | Combined (b) | 21.10 | 0.4% | 7.15 |
11.73 |
| XMM-Newton | 07/08/2008 | 0554920301 | 12.03 | < 1% | 9.12 |
12.07 |
| Chandra | 27/11/2010 | 12868 | 25.01 | < 0.1% | 4.10 |
21.18 |
| NuSTAR | 10/02/2016 | 60160087002 | 21.62 | 13% | – | 1.79 |
| NuSTAR | 05/01/2018 | 60301022002 | 27.05 | 17% | – | 2.04 |
| NuSTAR | 05/03/2018 | 60301022003 | 43.43 | 22% | – | 1.55 |
| Chandra | 05/05/2018 (c) | Combined (d) | 217.59 | < 0.1% | 0.92 |
1.99 |
| Swift-XRT | 24/05/2018 (e) | Combined (f) | 61.10 | 1.5% | 0.73 |
1.78 |
| NuSTAR | 17/07/2018 | 60301022005 | 41.84 | 17% | – | 2.02 |
| XMM-Newton | 23/07/2018 | 0821240201 | 56.57 | 2% | 1.10 |
2.16 |
| XMM-Newton | 04/01/2019 | 0821240301 | 24.19 | 3% | 0.51 |
1.02 |
Notes. The exposures of XMM are those after the filtering for the high flaring-background episodes and are the total times of all three cameras.
The combined observations are: 18789, 19560, 20366, 20367, 20368, 20369, 20370, 21432, 22082, 21433.
The combined observations are: 00080898001, 00080898002, 00088207001, 00088207002, 00088207003, 00035776002, 00035776003, 00035776004, 00035776005, 00035776006, 00035776007, 00035776008, 00035776010, 00035776011, 00035776012, 00035776014, 00035776015, 00035776016, 00035776017, 00035776018, 00035776019, 00035776020, 00035776021, 00035776023, 00035776024, 00035776025, 00035776026, 00035776027, 00035776029, 00035776031, 00035776032, 00035776033, 00035776034, 00035776035, 00035776036, 00035776037, 00035776038, 00035776039, 00035776040, 00035776041, 00035776042, 00035776043, 00035776044, 00035776045, 00035776046, 00035776047, 00035776049, 00035776050, 00035776051, 00035776052, 00035776054, 00035776055, 00035776056, 00035776057, 00035776058, 00035776059.
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