Table 2.
Open in new tab

Aperture photometry results of the XMM–Newton and NuSTAR observations in different energy bands.

DetectorGTI exposure timeNet countsCount rateNet countsCount rateNet countsCount rate
XMM–Newton(0.5–2 keV)(2–5 keV)(5–10 keV)
EPIC MOS-15202010 ± 51.8 × 10−4<10<2 × 10−4<10<2 × 10−4
EPIC MOS-2464006 ± 51.3 × 10−47 ± 41.6 × 10−4<11<2 × 10−4
EPIC PN4887015 ± 103.1 × 10−433 ± 96.8 × 10−4<24<5 × 10−4
NuSTAR(6–10 keV)(10–40 keV)(40–79 keV)
FPMA21860022 ± 91 × 10−425 ± 181 × 10−4<48<2 × 10−4
FPMB218600<31<1 × 10−4<54<3 × 10−4<45<2 × 10−4
DetectorGTI exposure timeNet countsCount rateNet countsCount rateNet countsCount rate
XMM–Newton(0.5–2 keV)(2–5 keV)(5–10 keV)
EPIC MOS-15202010 ± 51.8 × 10−4<10<2 × 10−4<10<2 × 10−4
EPIC MOS-2464006 ± 51.3 × 10−47 ± 41.6 × 10−4<11<2 × 10−4
EPIC PN4887015 ± 103.1 × 10−433 ± 96.8 × 10−4<24<5 × 10−4
NuSTAR(6–10 keV)(10–40 keV)(40–79 keV)
FPMA21860022 ± 91 × 10−425 ± 181 × 10−4<48<2 × 10−4
FPMB218600<31<1 × 10−4<54<3 × 10−4<45<2 × 10−4

Notes. XMM–Newton source counts were extracted from 15-arcsec apertures; and the NuSTAR source counts were extracted from 30-arcsec apertures. The EPIC detectors showed lower signal-to-noise ratio towards the harder bands compared to that of the PN detector. Of the two NuSTAR detectors, only FPMA showed real detections, so we show 3 σ upper limits for FPMB. The 3 σ upper limits are also shown for other bands with low counts. Only data from the EPIC and FPMA detectors were used for the spectral analysis. The   Good Time Interval (GTI) exposure time is in seconds.

Table 2.
Open in new tab

Aperture photometry results of the XMM–Newton and NuSTAR observations in different energy bands.

DetectorGTI exposure timeNet countsCount rateNet countsCount rateNet countsCount rate
XMM–Newton(0.5–2 keV)(2–5 keV)(5–10 keV)
EPIC MOS-15202010 ± 51.8 × 10−4<10<2 × 10−4<10<2 × 10−4
EPIC MOS-2464006 ± 51.3 × 10−47 ± 41.6 × 10−4<11<2 × 10−4
EPIC PN4887015 ± 103.1 × 10−433 ± 96.8 × 10−4<24<5 × 10−4
NuSTAR(6–10 keV)(10–40 keV)(40–79 keV)
FPMA21860022 ± 91 × 10−425 ± 181 × 10−4<48<2 × 10−4
FPMB218600<31<1 × 10−4<54<3 × 10−4<45<2 × 10−4
DetectorGTI exposure timeNet countsCount rateNet countsCount rateNet countsCount rate
XMM–Newton(0.5–2 keV)(2–5 keV)(5–10 keV)
EPIC MOS-15202010 ± 51.8 × 10−4<10<2 × 10−4<10<2 × 10−4
EPIC MOS-2464006 ± 51.3 × 10−47 ± 41.6 × 10−4<11<2 × 10−4
EPIC PN4887015 ± 103.1 × 10−433 ± 96.8 × 10−4<24<5 × 10−4
NuSTAR(6–10 keV)(10–40 keV)(40–79 keV)
FPMA21860022 ± 91 × 10−425 ± 181 × 10−4<48<2 × 10−4
FPMB218600<31<1 × 10−4<54<3 × 10−4<45<2 × 10−4

Notes. XMM–Newton source counts were extracted from 15-arcsec apertures; and the NuSTAR source counts were extracted from 30-arcsec apertures. The EPIC detectors showed lower signal-to-noise ratio towards the harder bands compared to that of the PN detector. Of the two NuSTAR detectors, only FPMA showed real detections, so we show 3 σ upper limits for FPMB. The 3 σ upper limits are also shown for other bands with low counts. Only data from the EPIC and FPMA detectors were used for the spectral analysis. The   Good Time Interval (GTI) exposure time is in seconds.

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