A dataset provided by the European Space Agency

Proposal ID 092414
Title Expanding a sample of X-ray confirmed intermediate-mass black holes
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DOI https://doi.org/10.57780/esa-huvg5ql
Principal Investigator, PI Dr Igor Chilingarian
Abstract Constraining the population of intermediate black holes (IMBHs) can help solveone of the long-standing problems in modern astrophysics, the origin ofsupermassive black holes (SMBHs). Among the 305 optically selected IMBHcandidates (3e4
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2023-10-20T16:45:54Z/2024-04-14T04:27:53Z
Version 21.51_20241115_1113
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 2025-04-27T00:00:00Z
Last Update 2026-07-09
Keywords XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Igor Chilingarian, 2025, 'Expanding a sample of X-ray confirmed intermediate-mass black holes', 21.51_20241115_1113, European Space Agency, https://doi.org/10.57780/esa-huvg5ql
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.