A dataset provided by the European Space Agency

Proposal ID 094253
Title Expanding a sample of X-ray confirmed intermediate-mass black holes
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DOI https://doi.org/10.57780/esa-e97np72
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 No publications found for current proposal!
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2024-06-20T01:39:22Z/2025-04-27T22:20:30Z
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 2026-05-31T00:00:00Z
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, 2026, 'Expanding a sample of X-ray confirmed intermediate-mass black holes', 21.51_20241115_1113, European Space Agency, https://doi.org/10.57780/esa-e97np72
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.