OBS_ID . | Date . | State . | Flux . | tRGS1, 2 . | tpn . | tMOS1 . | tMOS2 . | Notes . | Stacking . |
---|---|---|---|---|---|---|---|---|---|
. | . | . | (|$\rm {photons \, m}^{-2}\, \rm {s}^{-1}$|) . | (ks) . | (ks) . | (ks) . | (ks) . | . | group . |
0405090101 | 2006-10-15 | Low–Int | 7.8 | 97 | 81 | 99 | 99 | OLD L–I | |
0693850501 | 2012-12-16 | Low–Int | 10.1 | 112 | 90 | 114 | 113 | OLD L–I | |
0693851201 | 2012-12-22 | Low–Int | 11.0 | 117 | 85 | 122 | 121 | OLD L–I | |
0742590301 | 2014-07-05 | Int–Bright | 18.1 | 62 | 54 | 61 | 61 | (*) | |
0794580601 | 2017-03-29 | Low–Int | 11.0 | 41 | 26 | 39 | 37 | (*) | |
0803990101 | 2017-06-14 | Int–Bright | 15.5 | 131 | 109 | 128 | 128 | NEW I–B | |
0803990201 | 2017-06-20 | Int–Bright | 13.5 | 130 | 111 | 129 | 128 | NEW I–B | |
0803990301 | 2017-08-31 | Low–Int | 8.6 | 109 | 42 | 70 | 64 | (**) | NEW L–I |
0803990401 | 2017-09-02 | Low–Int | 8.5 | 115 | 53 | 50 | 46 | (**) | NEW L–I |
0803990701 | 2017-09-24 | Low–Int | 9.1 | 121 | 11 | 10 | 10 | (***) | NEW L–I |
0803990501 | 2017-12-07 | Int–Bright | 12.0 | 90 | 60 | 89 | 86 | (**) | NEW I–B |
0803990601 | 2017-12-09 | Int–Bright | 14.7 | 109 | 71 | 117 | 116 | (**) | NEW I–B |
OBS_ID . | Date . | State . | Flux . | tRGS1, 2 . | tpn . | tMOS1 . | tMOS2 . | Notes . | Stacking . |
---|---|---|---|---|---|---|---|---|---|
. | . | . | (|$\rm {photons \, m}^{-2}\, \rm {s}^{-1}$|) . | (ks) . | (ks) . | (ks) . | (ks) . | . | group . |
0405090101 | 2006-10-15 | Low–Int | 7.8 | 97 | 81 | 99 | 99 | OLD L–I | |
0693850501 | 2012-12-16 | Low–Int | 10.1 | 112 | 90 | 114 | 113 | OLD L–I | |
0693851201 | 2012-12-22 | Low–Int | 11.0 | 117 | 85 | 122 | 121 | OLD L–I | |
0742590301 | 2014-07-05 | Int–Bright | 18.1 | 62 | 54 | 61 | 61 | (*) | |
0794580601 | 2017-03-29 | Low–Int | 11.0 | 41 | 26 | 39 | 37 | (*) | |
0803990101 | 2017-06-14 | Int–Bright | 15.5 | 131 | 109 | 128 | 128 | NEW I–B | |
0803990201 | 2017-06-20 | Int–Bright | 13.5 | 130 | 111 | 129 | 128 | NEW I–B | |
0803990301 | 2017-08-31 | Low–Int | 8.6 | 109 | 42 | 70 | 64 | (**) | NEW L–I |
0803990401 | 2017-09-02 | Low–Int | 8.5 | 115 | 53 | 50 | 46 | (**) | NEW L–I |
0803990701 | 2017-09-24 | Low–Int | 9.1 | 121 | 11 | 10 | 10 | (***) | NEW L–I |
0803990501 | 2017-12-07 | Int–Bright | 12.0 | 90 | 60 | 89 | 86 | (**) | NEW I–B |
0803990601 | 2017-12-09 | Int–Bright | 14.7 | 109 | 71 | 117 | 116 | (**) | NEW I–B |
Notes. The ULX state refers to the low-to-intermediate and intermediate-to-bright flux levels, primarily chosen from the total flux and shape of the X-ray spectra (see Figs 2 and A1). Absorbed 0.3–10 keV fluxes are computed with a multicomponent model consisting of two modified blackbody components plus comptonization corrected for Galactic absorption (see Section 3.1). Exposure times account for background flaring removal. (*) RGS spectra contaminated by either X-2 or SNR (only EPIC-pn is used for PCA); (**) EPIC cameras affected by solar flares; (***) Additional calibration exposure (only RGS is operating for the full orbit).The acronyms OLD L–I, NEW L–I, and NEW I–B stay for old low–intermediate, new low–intermediate, and new intermediate–bright states.
OBS_ID . | Date . | State . | Flux . | tRGS1, 2 . | tpn . | tMOS1 . | tMOS2 . | Notes . | Stacking . |
---|---|---|---|---|---|---|---|---|---|
. | . | . | (|$\rm {photons \, m}^{-2}\, \rm {s}^{-1}$|) . | (ks) . | (ks) . | (ks) . | (ks) . | . | group . |
0405090101 | 2006-10-15 | Low–Int | 7.8 | 97 | 81 | 99 | 99 | OLD L–I | |
0693850501 | 2012-12-16 | Low–Int | 10.1 | 112 | 90 | 114 | 113 | OLD L–I | |
0693851201 | 2012-12-22 | Low–Int | 11.0 | 117 | 85 | 122 | 121 | OLD L–I | |
0742590301 | 2014-07-05 | Int–Bright | 18.1 | 62 | 54 | 61 | 61 | (*) | |
0794580601 | 2017-03-29 | Low–Int | 11.0 | 41 | 26 | 39 | 37 | (*) | |
0803990101 | 2017-06-14 | Int–Bright | 15.5 | 131 | 109 | 128 | 128 | NEW I–B | |
0803990201 | 2017-06-20 | Int–Bright | 13.5 | 130 | 111 | 129 | 128 | NEW I–B | |
0803990301 | 2017-08-31 | Low–Int | 8.6 | 109 | 42 | 70 | 64 | (**) | NEW L–I |
0803990401 | 2017-09-02 | Low–Int | 8.5 | 115 | 53 | 50 | 46 | (**) | NEW L–I |
0803990701 | 2017-09-24 | Low–Int | 9.1 | 121 | 11 | 10 | 10 | (***) | NEW L–I |
0803990501 | 2017-12-07 | Int–Bright | 12.0 | 90 | 60 | 89 | 86 | (**) | NEW I–B |
0803990601 | 2017-12-09 | Int–Bright | 14.7 | 109 | 71 | 117 | 116 | (**) | NEW I–B |
OBS_ID . | Date . | State . | Flux . | tRGS1, 2 . | tpn . | tMOS1 . | tMOS2 . | Notes . | Stacking . |
---|---|---|---|---|---|---|---|---|---|
. | . | . | (|$\rm {photons \, m}^{-2}\, \rm {s}^{-1}$|) . | (ks) . | (ks) . | (ks) . | (ks) . | . | group . |
0405090101 | 2006-10-15 | Low–Int | 7.8 | 97 | 81 | 99 | 99 | OLD L–I | |
0693850501 | 2012-12-16 | Low–Int | 10.1 | 112 | 90 | 114 | 113 | OLD L–I | |
0693851201 | 2012-12-22 | Low–Int | 11.0 | 117 | 85 | 122 | 121 | OLD L–I | |
0742590301 | 2014-07-05 | Int–Bright | 18.1 | 62 | 54 | 61 | 61 | (*) | |
0794580601 | 2017-03-29 | Low–Int | 11.0 | 41 | 26 | 39 | 37 | (*) | |
0803990101 | 2017-06-14 | Int–Bright | 15.5 | 131 | 109 | 128 | 128 | NEW I–B | |
0803990201 | 2017-06-20 | Int–Bright | 13.5 | 130 | 111 | 129 | 128 | NEW I–B | |
0803990301 | 2017-08-31 | Low–Int | 8.6 | 109 | 42 | 70 | 64 | (**) | NEW L–I |
0803990401 | 2017-09-02 | Low–Int | 8.5 | 115 | 53 | 50 | 46 | (**) | NEW L–I |
0803990701 | 2017-09-24 | Low–Int | 9.1 | 121 | 11 | 10 | 10 | (***) | NEW L–I |
0803990501 | 2017-12-07 | Int–Bright | 12.0 | 90 | 60 | 89 | 86 | (**) | NEW I–B |
0803990601 | 2017-12-09 | Int–Bright | 14.7 | 109 | 71 | 117 | 116 | (**) | NEW I–B |
Notes. The ULX state refers to the low-to-intermediate and intermediate-to-bright flux levels, primarily chosen from the total flux and shape of the X-ray spectra (see Figs 2 and A1). Absorbed 0.3–10 keV fluxes are computed with a multicomponent model consisting of two modified blackbody components plus comptonization corrected for Galactic absorption (see Section 3.1). Exposure times account for background flaring removal. (*) RGS spectra contaminated by either X-2 or SNR (only EPIC-pn is used for PCA); (**) EPIC cameras affected by solar flares; (***) Additional calibration exposure (only RGS is operating for the full orbit).The acronyms OLD L–I, NEW L–I, and NEW I–B stay for old low–intermediate, new low–intermediate, and new intermediate–bright states.
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