| Issue |
A&A
Volume 524, December 2010
|
|
|---|---|---|
| Article Number | A97 | |
| Number of page(s) | 13 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201015306 | |
| Published online | 25 November 2010 | |
Appendix A: Online material
Sources detected in the 0.3–7.5 keV energy band using PWDetect with detection threshold SNR = 5.
 |
Fig. A.1
X-ray spectra for known members of η Chamaleontis. Red is for EPIC-pn and black is for EPIC-mos, except for RECX 12 that is located in an EPIC-pn gap. The best fit to each spectrum is also plotted. The bottom panel represents the deviation of the model from the observed spectra in each spectral bin. |
| Open with DEXTER | |
 |
Fig. A.2
X-ray light curves in the energy band 0.3−8.0 keV for known members of η Chamaleontis. Time binning ranges from 15 to 30 min. |
| Open with DEXTER | |
© ESO, 2010
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