A dataset provided by the European Space Agency

Name 050501
Title X-ray study of the low black hole mass end of the AGN population with IMBH
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505010101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505010401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505010501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505011101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505011201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505011301

DOI https://doi.org/10.5270/esa-bms2y39
Author European Space Agency
Description Intermediate mass black hole (IMBH) are important in studies of black hole and
AGN physics and cosmology, but little is known about IMBH as a population due to
their rarity, especially in the X-ray band. We propose to observe with XMM a
well defined, volume limited, nearest (within 250Mpc) sample of IMBH AGN with
the least nominal black hole masses known so far (<3 10^5 M_sun) estimated using
the linewidth-luminosity-mass relation, which are discovered in our recent work.
XMM will enable detailed studies of X-ray spectral and temporal properties for
such objects both individually and as a sample extending up to 10keV energy
range, and will double the size of IMBH AGN with X-ray spectra to about two
dozens.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-06-19T15:40:37Z/2008-02-20T18:59:32Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2009-04-15T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009, X-Ray Study Of The Low Black Hole Mass End Of The Agn Population With Imbh, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-bms2y39