Searching for X-ray counterparts of unassociated Fermi-LAT sources and rotation-powered pulsars with SRG/eROSITA · arXivDesk
2401.17295Jan 30, 202416+5 pages, 11+3 figures, 4+4 tables; Abstract abridged; Accepted for publication in A&A; Part of the SRG/eROSITA DR1 paper splash
Searching for X-ray counterparts of unassociated Fermi-LAT sources and rotation-powered pulsars with SRG/eROSITA
The latest source catalog of the Fermi-LAT telescope contains more than 7000 γ-ray sources at GeV energies, with the two dominant source classes thought to be blazars and rotation-powered pulsars. Our target is the identification of possible (young and recycled) pulsar candidates in the sample of 2600 unassociated γ-ray sources, via their characteristic X-ray and γ-ray emission. To achieve this, we cross-match the Fermi-LAT catalog with the catalog of X-ray sources in the western Galactic hemisphere from the first four all-sky surveys of SRG/eROSITA. We complement this by identifying X-ray counterparts of known pulsars detected at γ-ray and radio energies in the eROSITA data. We use a Bayesian cross-matching scheme to construct a probabilistic catalog of possible pulsar-type X-ray counterparts to Fermi-LAT sources. Our method combines the overlap of X-ray and γ
Nearby in the stack
-ray source positions with a probabilistic classification (into pulsar and blazar candidates) of each source based on its
γ
-ray properties and a prediction on the X-ray flux of pulsar- or blazar-type counterparts. We provide a catalog of our prior
γ
-ray-based classifications of all 2600 unassociated sources in the Fermi-LAT catalog, with around equal numbers of pulsar and blazar candidates. Our final list of candidate X-ray pulsar counterparts, cleaned for spurious detections and sources with obvious non-pulsar counterparts, contains around 900 X-ray sources. We predict between 30 and 40 new pulsars among our top 200 candidates, with around equal expected numbers of young and recycled pulsars. This candidate list may serve as input to future follow-up campaigns, looking directly for pulsations or for the orbital modulation of possible binary companions. We furthermore detect the X-ray counterparts of 15 known rotation-powered pulsars, which were not seen in X-rays before.
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