| Telescope . | Observation . | Observation . | Exposure . | |$F_{\mathrm{0.3-10}}$| . | Joint . |
|---|---|---|---|---|---|
| . | date . | ID . | time (s) . | (10|$^{-12}$| erg cm|$^{-2}$| s|$^{-1}$|) . | data set . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . |
| XMM–Newton | 2002-01-01 | 0109130301 | 11349 | 8.6 | |
| 2004-07-04 | 0201020201 | 112674 | 11.3 | ||
| 2020-07-04 | 0865470201 | 27000 | 10.8 | ||
| 2021-01-03 | 0865470301 | 27000 | 12.6 | J21 | |
| 2021-08-11 | 0870840101, 0870840401 | 17998 | 18.8 | HF | |
| 2022-01-24 | 0870840201 | 25800 | 3.8 | LF | |
| 2022-07-28 | 0912400101 | 27000 | 9.3 | ||
| 2023-02-06 | 0870840301 | 38000 | 6.8 | LF; F23 | |
| 2024-01-25 | 0912400201 | 27000 | 21.5 | HF | |
| NuSTAR | 2016-02-05 | 60160095002 | 21205 | 4.9 | LF |
| 2016-12-02 | 90201043002 | 51001 | 5.0 | LF | |
| 2018-10-27 | 80402610002 | 21069 | 14.8 | ||
| 2019-08-31 | 80502630002 | 68123 | 21.8 | HF | |
| 2020-01-21 | 80502630004 | 50168 | 20.9 | HF | |
| 2021-01-10 | 80502630006 | 41517 | 10.9 | J21 | |
| 2021-08-18 | 60761012002 | 18649 | 22.1 | HF | |
| 2021-12-22 | 80602604002 | 53311 | 8.4 | ||
| 2023-02-06 | 80602604004 | 40977 | 8.0 | F23 | |
| 2023-09-29 | 80802652002 | 20825 | 5.5 | LF | |
| 2024-01-25 | 80802652004 | 62046 | 24.7 | HF | |
| NICER | 2022-07-16 | 5667010401 | 1743 | 9.6 | |
| 2022-07-26 | 5667010501 | 3371 | 10.4 | ||
| 2022-08-15 | 5667010702 | 2052 | 14.7 | ||
| 2022-08-24 | 5667010801 | 1015 | 8.0 | ||
| 2022-08-25 | 5667010802 | 2043 | 7.7 | ||
| 2022-09-14 | 5667011001 | 2636 | 9.9 | ||
| 2022-09-25 | 5667011101 | 2522 | 8.7 | ||
| 2022-10-04 | 5667011201 | 1786 | 17.6 | ||
| 2022-10-24 | 5667011401 | 1917 | 6.1 | ||
| 2022-11-12 | 5667011601 | 1815 | 6.2 | ||
| 2022-12-03 | 5667011801 | 1505 | 5.2 | ||
| 2023-01-08 | 5667012101 | 3498 | 5.0 |
| Telescope . | Observation . | Observation . | Exposure . | |$F_{\mathrm{0.3-10}}$| . | Joint . |
|---|---|---|---|---|---|
| . | date . | ID . | time (s) . | (10|$^{-12}$| erg cm|$^{-2}$| s|$^{-1}$|) . | data set . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . |
| XMM–Newton | 2002-01-01 | 0109130301 | 11349 | 8.6 | |
| 2004-07-04 | 0201020201 | 112674 | 11.3 | ||
| 2020-07-04 | 0865470201 | 27000 | 10.8 | ||
| 2021-01-03 | 0865470301 | 27000 | 12.6 | J21 | |
| 2021-08-11 | 0870840101, 0870840401 | 17998 | 18.8 | HF | |
| 2022-01-24 | 0870840201 | 25800 | 3.8 | LF | |
| 2022-07-28 | 0912400101 | 27000 | 9.3 | ||
| 2023-02-06 | 0870840301 | 38000 | 6.8 | LF; F23 | |
| 2024-01-25 | 0912400201 | 27000 | 21.5 | HF | |
| NuSTAR | 2016-02-05 | 60160095002 | 21205 | 4.9 | LF |
| 2016-12-02 | 90201043002 | 51001 | 5.0 | LF | |
| 2018-10-27 | 80402610002 | 21069 | 14.8 | ||
| 2019-08-31 | 80502630002 | 68123 | 21.8 | HF | |
| 2020-01-21 | 80502630004 | 50168 | 20.9 | HF | |
| 2021-01-10 | 80502630006 | 41517 | 10.9 | J21 | |
| 2021-08-18 | 60761012002 | 18649 | 22.1 | HF | |
| 2021-12-22 | 80602604002 | 53311 | 8.4 | ||
| 2023-02-06 | 80602604004 | 40977 | 8.0 | F23 | |
| 2023-09-29 | 80802652002 | 20825 | 5.5 | LF | |
| 2024-01-25 | 80802652004 | 62046 | 24.7 | HF | |
| NICER | 2022-07-16 | 5667010401 | 1743 | 9.6 | |
| 2022-07-26 | 5667010501 | 3371 | 10.4 | ||
| 2022-08-15 | 5667010702 | 2052 | 14.7 | ||
| 2022-08-24 | 5667010801 | 1015 | 8.0 | ||
| 2022-08-25 | 5667010802 | 2043 | 7.7 | ||
| 2022-09-14 | 5667011001 | 2636 | 9.9 | ||
| 2022-09-25 | 5667011101 | 2522 | 8.7 | ||
| 2022-10-04 | 5667011201 | 1786 | 17.6 | ||
| 2022-10-24 | 5667011401 | 1917 | 6.1 | ||
| 2022-11-12 | 5667011601 | 1815 | 6.2 | ||
| 2022-12-03 | 5667011801 | 1505 | 5.2 | ||
| 2023-01-08 | 5667012101 | 3498 | 5.0 |
Note. All parameter uncertainties are quoted at the 90th percentile confidence interval. (1) Telescope name. (2) Date of observation start, YYYY-MM-DD. (3) Observation identifier in the HEASarc archive. (4) On-source integration time. This is measured before event screening. (5) Integrated 0.3–10 keV model flux, determined using the phenomenological model (Section 3.2). As NuSTAR is not sensitive below 3 keV, the best-fitting model is extrapolated, to facilitate comparison with the other telescopes. (6) Data set(s) that this observation is included in for the joint analysis described in Section 3.3.
| Telescope . | Observation . | Observation . | Exposure . | |$F_{\mathrm{0.3-10}}$| . | Joint . |
|---|---|---|---|---|---|
| . | date . | ID . | time (s) . | (10|$^{-12}$| erg cm|$^{-2}$| s|$^{-1}$|) . | data set . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . |
| XMM–Newton | 2002-01-01 | 0109130301 | 11349 | 8.6 | |
| 2004-07-04 | 0201020201 | 112674 | 11.3 | ||
| 2020-07-04 | 0865470201 | 27000 | 10.8 | ||
| 2021-01-03 | 0865470301 | 27000 | 12.6 | J21 | |
| 2021-08-11 | 0870840101, 0870840401 | 17998 | 18.8 | HF | |
| 2022-01-24 | 0870840201 | 25800 | 3.8 | LF | |
| 2022-07-28 | 0912400101 | 27000 | 9.3 | ||
| 2023-02-06 | 0870840301 | 38000 | 6.8 | LF; F23 | |
| 2024-01-25 | 0912400201 | 27000 | 21.5 | HF | |
| NuSTAR | 2016-02-05 | 60160095002 | 21205 | 4.9 | LF |
| 2016-12-02 | 90201043002 | 51001 | 5.0 | LF | |
| 2018-10-27 | 80402610002 | 21069 | 14.8 | ||
| 2019-08-31 | 80502630002 | 68123 | 21.8 | HF | |
| 2020-01-21 | 80502630004 | 50168 | 20.9 | HF | |
| 2021-01-10 | 80502630006 | 41517 | 10.9 | J21 | |
| 2021-08-18 | 60761012002 | 18649 | 22.1 | HF | |
| 2021-12-22 | 80602604002 | 53311 | 8.4 | ||
| 2023-02-06 | 80602604004 | 40977 | 8.0 | F23 | |
| 2023-09-29 | 80802652002 | 20825 | 5.5 | LF | |
| 2024-01-25 | 80802652004 | 62046 | 24.7 | HF | |
| NICER | 2022-07-16 | 5667010401 | 1743 | 9.6 | |
| 2022-07-26 | 5667010501 | 3371 | 10.4 | ||
| 2022-08-15 | 5667010702 | 2052 | 14.7 | ||
| 2022-08-24 | 5667010801 | 1015 | 8.0 | ||
| 2022-08-25 | 5667010802 | 2043 | 7.7 | ||
| 2022-09-14 | 5667011001 | 2636 | 9.9 | ||
| 2022-09-25 | 5667011101 | 2522 | 8.7 | ||
| 2022-10-04 | 5667011201 | 1786 | 17.6 | ||
| 2022-10-24 | 5667011401 | 1917 | 6.1 | ||
| 2022-11-12 | 5667011601 | 1815 | 6.2 | ||
| 2022-12-03 | 5667011801 | 1505 | 5.2 | ||
| 2023-01-08 | 5667012101 | 3498 | 5.0 |
| Telescope . | Observation . | Observation . | Exposure . | |$F_{\mathrm{0.3-10}}$| . | Joint . |
|---|---|---|---|---|---|
| . | date . | ID . | time (s) . | (10|$^{-12}$| erg cm|$^{-2}$| s|$^{-1}$|) . | data set . |
| (1) . | (2) . | (3) . | (4) . | (5) . | (6) . |
| XMM–Newton | 2002-01-01 | 0109130301 | 11349 | 8.6 | |
| 2004-07-04 | 0201020201 | 112674 | 11.3 | ||
| 2020-07-04 | 0865470201 | 27000 | 10.8 | ||
| 2021-01-03 | 0865470301 | 27000 | 12.6 | J21 | |
| 2021-08-11 | 0870840101, 0870840401 | 17998 | 18.8 | HF | |
| 2022-01-24 | 0870840201 | 25800 | 3.8 | LF | |
| 2022-07-28 | 0912400101 | 27000 | 9.3 | ||
| 2023-02-06 | 0870840301 | 38000 | 6.8 | LF; F23 | |
| 2024-01-25 | 0912400201 | 27000 | 21.5 | HF | |
| NuSTAR | 2016-02-05 | 60160095002 | 21205 | 4.9 | LF |
| 2016-12-02 | 90201043002 | 51001 | 5.0 | LF | |
| 2018-10-27 | 80402610002 | 21069 | 14.8 | ||
| 2019-08-31 | 80502630002 | 68123 | 21.8 | HF | |
| 2020-01-21 | 80502630004 | 50168 | 20.9 | HF | |
| 2021-01-10 | 80502630006 | 41517 | 10.9 | J21 | |
| 2021-08-18 | 60761012002 | 18649 | 22.1 | HF | |
| 2021-12-22 | 80602604002 | 53311 | 8.4 | ||
| 2023-02-06 | 80602604004 | 40977 | 8.0 | F23 | |
| 2023-09-29 | 80802652002 | 20825 | 5.5 | LF | |
| 2024-01-25 | 80802652004 | 62046 | 24.7 | HF | |
| NICER | 2022-07-16 | 5667010401 | 1743 | 9.6 | |
| 2022-07-26 | 5667010501 | 3371 | 10.4 | ||
| 2022-08-15 | 5667010702 | 2052 | 14.7 | ||
| 2022-08-24 | 5667010801 | 1015 | 8.0 | ||
| 2022-08-25 | 5667010802 | 2043 | 7.7 | ||
| 2022-09-14 | 5667011001 | 2636 | 9.9 | ||
| 2022-09-25 | 5667011101 | 2522 | 8.7 | ||
| 2022-10-04 | 5667011201 | 1786 | 17.6 | ||
| 2022-10-24 | 5667011401 | 1917 | 6.1 | ||
| 2022-11-12 | 5667011601 | 1815 | 6.2 | ||
| 2022-12-03 | 5667011801 | 1505 | 5.2 | ||
| 2023-01-08 | 5667012101 | 3498 | 5.0 |
Note. All parameter uncertainties are quoted at the 90th percentile confidence interval. (1) Telescope name. (2) Date of observation start, YYYY-MM-DD. (3) Observation identifier in the HEASarc archive. (4) On-source integration time. This is measured before event screening. (5) Integrated 0.3–10 keV model flux, determined using the phenomenological model (Section 3.2). As NuSTAR is not sensitive below 3 keV, the best-fitting model is extrapolated, to facilitate comparison with the other telescopes. (6) Data set(s) that this observation is included in for the joint analysis described in Section 3.3.
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