A dataset provided by the European Space Agency

Name 088377
Title A systematic search for X-ray Quasi-Periodic Eruptions in the eROSITA era
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883770901

DOI https://doi.org/10.57780/esa-wat5pc9
Author European Space Agency
Description QPEs are extreme soft X-ray bursts recurring on hours timescales associated to
low-z galactic nuclei. Until a few months ago, only two such sources were found
and currently the only way of systematically finding new QPEs is provided by
SRG/eROSITA. In AO19 we were able to discover, in synergy with XMM-Newton, two
new QPEs. Thanks to this pilot study, we are now confident in finding 3-4 good
candidates every year. We plan to use 1-1.5yrs of eROSITA data to trigger
XMM-Newton during AO20, therefore we ask for 4 ToO observations to be performed
on 4 different candidates, each with a length of 130 ks. By the end of AO20 this
synergy can double the number of the now 4 known QPEs, which will allow us to
better understand and characterise these new and interesting phenomena.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-06-21T16:29:57Z/2023-03-11T12:56:52Z
Version 20.10_20230417_1156
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2024-04-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2024, A Systematic Search For X-Ray Quasi-Periodic Eruptions In The Erosita Era, 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-wat5pc9