Table 5: Log of archival and present observations of WR 25.
obs. instrument observation MJDa exposure total duration
no.   ID date   (s) (s)
1 ROSAT- PSPCB rp200108n00 1991, Dec. 15 48605.41 1610  2839
2 ROSAT- PSPCB rp900176n00 1992, Jun. 12 48785.94 24 321  225 050
3 ROSAT- PSPCB rp201262n00 1992, Aug. 09 48843.93 5665  42 858
4 ROSAT- PSPCB rp900176a01 1992, Dec. 15 48971.73 14 544  2 096 652
5 ASCA- SIS0+SIS1 20018000 1993, Aug. 24 49223.76 30 048  74260
6 ASCA- SIS0+SIS1 26033000 1997, Jan. 24 50806.90 37 712  113 184
7 XMM-Newton- MOS1+PNb 0112580601 2000, Jul. 26 51751.71 31 600c 36 604
8 XMM-Newton- MOS1+PNb 0112580701 2000, Jul. 27 51753.50 9700c 12 572
9 XMM-Newton- MOS1+MOS2+PN 0112560101 2001, Jun. 25 52085.79 23 900c 36 994
10 XMM-Newton- MOS1+MOS2+PN 0112560201 2001, Jun. 28 52088.81 27 500c 38 506
11 XMM-Newton- MOS1+MOS2+PN 0112560301 2001, Jun. 30 52090.70 32 600c 37 474
12 XMM-Newton- RGS1+RGS2+MOS1 0112560201 2001, Jun. 28 52088.81 25 300c 38 506
13 XMM-Newton- RGS1+RGS2+MOS1 0112560301 2001, Jun. 30 52090.70 33 300c 37 474
a Exposure start.
b MOS2 was in "small window mode'', with WR 25 close to the edge of the central CCD, which renders the data unusable.
c Some exposure time was lost due to (solar) high soft proton rate. Average exposure time is shown here, individual exposures
for MOS1, MOS2, PN, RGS1, RGS2 are slightly different.


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