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Table 1

IC 3599 X-ray observation log.

Instrument Obs. ID. Obs. start Duration (ks) Counts* Spectrum

ROSAT/RASS rs931231n00 1990-12-10 0.8
ROSAT/PSPC rp700552a00 1991-12-15 3.3 101 ± 11 1
ROSAT/PSPC rp700552a01 1992-05-31 1.4 33 ± 6 2
ROSAT/PSPC rp701098n00 1992-06-16 1.8 36 ± 6 2
ROSAT/PSPC rp701099n00 1992-06-17 1.9 33 ± 6 2
ROSAT/PSPC rp701100n00 1992-06-18 2.0 36 ± 6 2
ROSAT/PSPC rp701097n00 1992-06-30 5.4 116 ± 12 3
ROSAT/PSPC rp701528n00 1993-06-17 3.4 26 ± 5 3
ROSAT/HRI rh702704n00 1996-06-30 14.7 77 ± 11 3
ROSAT/HRI rh702706n00 1996-06-30 16.9 87 ± 12 3
Chandra/ACIS-S acisf029999N003 2002-03-07 10.6 427 ± 21 4
Swift/XRT 00037507001 2010-02-25 2.1 432 ± 23 5
Swift/XRT 00037507003 2010-05-17 1.2 100 ± 11 6
Swift/XRT 00037507004 2013-10-30 4.8 21 ± 6 7
Swift/XRT 00037507005 2013-11-06 4.9 12 ± 4 7
Swift/XRT 00037507006 2014-03-26 4.7 14 ± 4 7
Swift/XRT 00037569001 2014-08-08 1.6 <16
Swift/XRT 00037569001 2014-11-15 4.6 18 ± 5 7
Swift/XRT 00037569001 2014-11-23 0.4 <38

Notes.

(*)

The total number of counts was determined using the XIMAGE (v. 4.5.1) task detect (correcting for vignetting and point spread function losses). Spectra were grouped according to the scheme that spectra with the same number were grouped together. Numbers in italics mean that we used that given conversion factor to pass from count rates to fluxes even if no spectra analysis was carried out on these data because there were too few counts. Two ROSAT/PSPC observations on 1992-06-30 and 1992-12-08 were not considered because IC 3599 is too far off-axis to be detected.

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