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

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

DOI 10.5270/esa-bms2y39
Author Dr Weimin Yuan
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 A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 . Georgakakis, Antonis, Nandra, K., . MNRAS . 414-992 . 2011 . 2011MNRAS.414..992G ,
X-Ray Spectral Curvature of High-frequency-peaked BL Lac Objects: A Predictor for the TeV Flux . Massaro, F., Paggi, A., et all. . ApJ . 739-73 . 2011 . 2011ApJ...739...73M ,
XMM-Newton and Swift observations of High Frequency Peaked BL Lacs in the TeV era . Massaro, F., Paggi, A., et all. . JPhCS . 355-12012 . 2012 . 2012JPhCS.355a2012M ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
The X-ray luminous galaxies optically classified as star forming are mostly narrow line Seyfert 1 s . Castello-Mor, N., Barcons, X., et all. . A&A . 544-48 . 2012 . 2012A&A...544A..48C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ...
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, 2009-04-15T00:00:00Z, 050501, 17.56_20190403_1200. https://doi.org/10.5270/esa-bms2y39