A dataset provided by the European Space Agency

Proposal ID 067481
Title A survey of intermediate mass black holes in dwarf AGN
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DOI https://doi.org/10.5270/esa-l4u6gnx
Principal Investigator, PI Dr Edward Cackett
Abstract Black holes are seen over a huge range in mass in the Universe, ranging fromstellar-mass black holes in binary systems, to supermassive (1E6 - 1E9 M(sun))black holes at the centers of AGN. The recent discovery of low luminosity AGNwith black hole masses less than 1E6 M(sun) allows a unique probe of theproperties of accretion onto intermediate mass black holes. Only 6 of theseobjects have had previous significant X-ray observations, and have showntantalising evidence of extreme variability and even a soft excess. Here, wepropose to survey the 8 remaining objects with a mass less than 1E6 M(sun) andknown X-ray counterpart, more than doubling the sample of good X-rayobservations of these objects.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-05-03T17:07:10Z/2012-01-17T19:26:25Z
Version 17.56_20190403_1200
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 2013-02-14T00:00:00Z
Keywords "soft excess", "blackhole masses", "xray counterpart", "huge range", "1e6 msun", "binary systems", "stellar mass blackhole", "tantalising evidence", "dwarf agn", "1e6 msun allows", "low luminosity agn", "intermediate mass blackhole"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Edward Cackett, 2013, 'A survey of intermediate mass black holes in dwarf AGN', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-l4u6gnx