eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866929665068761088 |
|---|---|
| author | Grotova, Iuliia Rau, Arne Salvato, Mara Buchner, Johannes Goodwin, Adelle J. Liu, Zhu Malyali, Adam Merloni, Andrea Tubín-Arenas, Dusán Homan, David Krumpe, Mirko Nandra, Kirpal Anderson, Gemma E. Arcodia, Riccardo Bahic, Sabina Baldini, Pietro Buckley, David A. H. Ciroi, Stefano Kawka, Adela Masterson, Megan Miller-Jones, James C. A. Di Mille, Francesco |
| author_facet | Grotova, Iuliia Rau, Arne Salvato, Mara Buchner, Johannes Goodwin, Adelle J. Liu, Zhu Malyali, Adam Merloni, Andrea Tubín-Arenas, Dusán Homan, David Krumpe, Mirko Nandra, Kirpal Anderson, Gemma E. Arcodia, Riccardo Bahic, Sabina Baldini, Pietro Buckley, David A. H. Ciroi, Stefano Kawka, Adela Masterson, Megan Miller-Jones, James C. A. Di Mille, Francesco |
| contents | (Abridged) While previous X-ray studies showed the dominance of regular active galactic nuclei (AGN) variability, a small fraction of sources arise from more exotic phenomena such as tidal disruption events (TDEs), quasi-periodic eruptions, or other short-lived events associated with supermassive black hole accretion. This paper describes the systematic selection of X-ray extragalactic transients found in the first two eROSITA all-sky surveys (eRASS) that are not associated with known AGN prior to eROSITA observations. We generated a variability sample from eRASS1 and eRASS2 (Dec. 2019-Dec. 2020), which includes sources with a variability significance and a fractional amplitude larger than four, located in the Legacy Survey DR10 (LS10) footprint. The properties of LS10 counterparts were used to exclude stars and known AGN. The sample was additionally cleaned using pre-eROSITA classifications, archival optical spectra, and archival X-ray data. The final catalog eRO-ExTra includes 304 extragalactic eROSITA transients and variables not associated with known AGN. More than 90% of sources have reliable LS10 optical counterparts. For each source, we provide archival X-ray data from Swift, ROSAT, and XMM-Newton; the eROSITA long-term light curve (2-2.5 years) with a light curve classification; as well as the best power law fit spectral results at the peak eROSITA epoch. Reliable spectroscopic and photometric redshifts are provided for more than 80% of the sample. Several sources in the catalog are known TDE candidates discovered by eROSITA. In addition, 31 sources are radio detected. The eRO-ExTra transients constitute a relatively clean parent sample of non-AGN variability phenomena associated with massive black holes. More than 95% of eRO-ExTra sources were discovered in X-rays with eROSITA for the first time, which makes it a valuable resource for studying unique nuclear transients. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_04208 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2 Grotova, Iuliia Rau, Arne Salvato, Mara Buchner, Johannes Goodwin, Adelle J. Liu, Zhu Malyali, Adam Merloni, Andrea Tubín-Arenas, Dusán Homan, David Krumpe, Mirko Nandra, Kirpal Anderson, Gemma E. Arcodia, Riccardo Bahic, Sabina Baldini, Pietro Buckley, David A. H. Ciroi, Stefano Kawka, Adela Masterson, Megan Miller-Jones, James C. A. Di Mille, Francesco High Energy Astrophysical Phenomena (Abridged) While previous X-ray studies showed the dominance of regular active galactic nuclei (AGN) variability, a small fraction of sources arise from more exotic phenomena such as tidal disruption events (TDEs), quasi-periodic eruptions, or other short-lived events associated with supermassive black hole accretion. This paper describes the systematic selection of X-ray extragalactic transients found in the first two eROSITA all-sky surveys (eRASS) that are not associated with known AGN prior to eROSITA observations. We generated a variability sample from eRASS1 and eRASS2 (Dec. 2019-Dec. 2020), which includes sources with a variability significance and a fractional amplitude larger than four, located in the Legacy Survey DR10 (LS10) footprint. The properties of LS10 counterparts were used to exclude stars and known AGN. The sample was additionally cleaned using pre-eROSITA classifications, archival optical spectra, and archival X-ray data. The final catalog eRO-ExTra includes 304 extragalactic eROSITA transients and variables not associated with known AGN. More than 90% of sources have reliable LS10 optical counterparts. For each source, we provide archival X-ray data from Swift, ROSAT, and XMM-Newton; the eROSITA long-term light curve (2-2.5 years) with a light curve classification; as well as the best power law fit spectral results at the peak eROSITA epoch. Reliable spectroscopic and photometric redshifts are provided for more than 80% of the sample. Several sources in the catalog are known TDE candidates discovered by eROSITA. In addition, 31 sources are radio detected. The eRO-ExTra transients constitute a relatively clean parent sample of non-AGN variability phenomena associated with massive black holes. More than 95% of eRO-ExTra sources were discovered in X-rays with eROSITA for the first time, which makes it a valuable resource for studying unique nuclear transients. |
| title | eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2 |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2501.04208 |