| Proposal ID | 088346 |
| Title | Follow-up of X-ray binary candidates in eRosita survey. |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0883460101 |
| DOI | https://doi.org/10.57780/esa-42tkh0v |
| Principal Investigator, PI | Dr Victor Doroshenko |
| Abstract | The ongoing eRosita survey (eRASS) is expected to discover several millions ofnew X-ray sources and double the number of known Galactic X-ray binaries (XRBs).This will help to clarify several long-standing questions related to theaccretion physics in low-luminosity XRB, their numbers, origin, and evolution.To fully realise this potential, follow-up observations in X-ray and other bandsare, however, essential. Here we propose to start the exploration of this newexciting dataset with XMM-Newton and follow-up several new High mass X-raybinary (HMXB) candidates identified with Rosita in order to confirm preliminaryidentification and study their X-ray properties in detail. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2021-09-14T03:57:37Z/2022-02-25T09:56:03Z |
| Version | 19.17_20220121_1250 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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 | 2023-03-12T00:00:00Z |
| Keywords | "erosita survey erass", "xray properties", "xray sources", "accretion physics", "XMM", "exciting dataset", "XMM-Newton", "preliminary identification", "low luminosity xrb", "xray binary candidates", "erosita survey ..", "xmm newton" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Victor Doroshenko, 2023, 'Follow-up of X-ray binary candidates in eRosita survey.', 19.17_20220121_1250, European Space Agency, https://doi.org/10.57780/esa-42tkh0v |