XMM spectra of eruptions and quiescence used in the paper titled "Alive and Strongly Kicking: Stable X-ray Quasi-Periodic Eruptions from eRO-QPE2 over 3.5 Years"
<p>The gz file has a folder containing 10 sets of spectra (two per XMMID: one using data from eruptions and one from quiescence). Each one has a corresponding rmf, arf and a background file.</p> <p>The files of the format: <span>PN_Grouped_spectrumXX...fits are xspec ready. They are grouped with specgroup task of XMMSAS with mincounts=1 oversample=3. Thus, cstat is recommended while fitting in XSPEC.</span></p> <p><span>Alternatively, the original source spectra (</span><span>PN_SPEC_SRCBKGXXX...fits) are also available so that the user can bin them as per their requirement.</span></p> <p><span>The background spectra have the following naming sequence: </span><span>PN_SPEC_BKGXX</span></p> <p> </p> <p><span>XX = "hi" ==> eruption spectra</span></p> <p><span>XX = "low" ==> quiescence spectra</span></p> <p><span>The numbers 1...5 correspond to XMM obsIDs as follows:</span></p> <p><span>1: </span><span>0872390101</span></p> <p><span>2: 0883770201</span></p> <p><span>3: 0893810501</span></p> <p><span>4: 0932590101</span></p> <p><span>5: 0932590201</span></p> <p> </p>
ShareScore
32/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 4
- Harmonization
- 4
- Access
- 16
- Reuse readiness
- 8
- Engagement
- 0