| Proposal ID | 088259 |
| Title | XMM Follow-Up of Tidal DIsruption Events in ZTF\\: Building a Legacy Sample |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0882590101 |
| DOI | https://doi.org/10.57780/esa-dvlmek3 |
| Principal Investigator, PI | Dr Suvi Gezari |
| Abstract | The Zwicky Transient Facility (ZTF) is on track to transform the field of tidaldisruption events (TDEs). In the first 2.5 yr of ZTF survey operations (ZTF-I),we have detected 25 TDEs. However, despite this exciting progress in assemblinga large sample of TDEs, the nature of the optical emission remains a mystery,and appears to be distinct from the soft X-ray component (kTvirgul50 eV) associatedwith the accretion of the stellar debris through a newly formed disk. In fact,with our X-ray follow-up observations we have revealed that the soft X-rays showdramatic variability that is totally decoupled from the smoothly evolvingoptical emission. Here propose for a program in AO-20 in order to create alegacy sample for X-ray population studies of TDEs for the first time. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2021-08-04T01:46:14Z/2023-08-14T02:25:45Z |
| Version | 20.10_20230417_1156 |
| 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 | 2024-08-26T00:00:00Z |
| Keywords | "exciting progress", "XMM", "optical emission", "tidal disruption events", "xray population", "soft xray", "ztf \: building", "stellar debris", "formed disk", "totally decoupled" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Suvi Gezari, 2024, 'XMM Follow-Up of Tidal DIsruption Events in ZTF\\: Building a Legacy Sample', 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-dvlmek3 |