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Table A.1

X-ray observations of RX J0520.5-6932.

ObsID MJD Instrumenta Off-axis angleb Net exp Net count ratesc,d F x e
[Tstart] [′] [ks] [10-2 cts s-1] [erg s-1 cm-2]
XMM
0690750901 56 266.1 EPIC-pn 10.9 22.24 0.94±0.15 7 × 10-14
EPIC-MOS1 10.0 26.37 0.18±0.0006 –
EPIC-MOS2 10.5 26.39 0.14±0.0007 –
0701990101 56 314.0 EPIC-pn 1.1 16.82 101.4±0.8 6.0 × 10-12
EPIC-MOS1 0.17 20.3 33.6±0.5 –
EPIC-MOS2 1.2 20.31 33.3±0.4 –
Swift
00045467001 56 270.5 11.6 1.12 <1.0 < 7.7 × 10-13
00045478001 56 305.4 8.0 1.65 2.4±0.6 18.4 × 10-13
00032671001 56 306.8 2.3 1.97 1.7±0.4 13.1 × 10-13
00032671002 56 308.0 1.9 1.28 2.7±0.6 20.7 × 10-13
00045479001 56 309.3 7.2 0.70 3.3±1.0 25.4 × 10-13
00032671003 56 310.3 2.0 2.32 4.8±0.6 36.9 × 10-13
00045479002 56 312.0 8.6 2.91 8.6±0.8 66.1 × 10-13
00045478002 56 312.8 8.5 1.99 11.4±1.1 87.6 × 10-13
00032671004 56 315.2 3.7 2.12 10.8±1.0 83.0 × 10-13
00045478003 56 317.4 8.7 1.03 4.6±1.0 35.4 × 10-13
00032671005 56 319.2 2.3 1.84 2.0±0.4 15.4 × 10-13
00032671006 56 323.0 2.8 2.03 <0.4 < 3.1 × 10-13
00032671007 56 327.0 2.8 2.15 <0.32 < 2.5 × 10-13
00032671008 56 331.2 1.9 1.92 3.5±0.6 26.9 × 10-13
00032671009 56 354.2 0.07 2.21 0.61±0.23 4.7 × 10-13
00032671010 56 358.6 2.2 1.92 1.4±0.4 10.8 × 10-13
00032671011 56 362.2 0.6 2.02 <0.64 < 4.9 × 10-13
00032671012 56 366.1 2.9 1.82 <0.32 < 2.5 × 10-13
00032671013 56 370.2 2.1 2.30 <0.26 < 2.0 × 10-13
00032671014 56 374.6 1.7 1.85 <0.6 < 4.6 × 10-13
00032671015 56 378.5 2.9 0.249 <0.28 < 2.2 × 10-13
00032671016 56 382.1 0.6 2.17 1.1±0.3 8.5 × 10-13
00032671017 56 406.0 1.3 2.00 5.87±0.23 45.1 × 10-13
00032671019 56 412.3 2.0 2.12 <0.4 < 3.1 × 10-13
00032671020 56 430.5 0.7 1.00 <0.53 < 4.1 × 10-13
00032671021 56 433.0 3.0 1.85 <0.38 < 2.9 × 10-13
00032671022 56 436.0 2.2 2.16 <0.35 < 2.7 × 10-13

Notes.

(a)

Observation setup for XMM-Newton: EPIC-pn in full-frame mode with thin filter, EPIC-MOS in full-frame mode with medium filter. All Swift observations are made with XRT instrument in photon-counting mode.

(b)

The off-axis angle of individual detections given (′).

(c)

Net count rate for the 0.3–10.0 keV band of XMM-Newton.

(d)

Swift/XRT count rates in the 0.3–10.0 keV band corrected for telescope vignetting. For the non-detections we list the 2σ upper limits.

(e)

X-ray observed flux in the 0.3–10.0 keV band, derived from the best fit spectral model. The Swift fluxes were derived from the XRT count rates assuming the best-fit absorbed power-law model derived from the XMM-Newton ToO spectra.

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