A dataset provided by the European Space Agency

Name 012370
Title An XMM PV survey of the Lockman Hole
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123700101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123700201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123700401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123700701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123700901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0123701001

DOI 10.5270/esa-s1pl1sx
Author Dr Fred Jansen XMM-Newton PS
Description The Lockman Hole provides the deepest X-ray survey done with ROSAT. About 80 X-ray sources have been uniquely optically identified. It is also covered by deep Radio-, ISO-, ASCA- adn Beppo-SAX surveys. With 150 ksec XMM PV observation, small systematics errors in the attitude solution, the platescale, systematic position errors and the point-spread function can all be measured. This will also give the first experimental determination of the XMM opportunity to identify confusion limit. This multi wavelength dataset will also provide a unique opportunity to identify the population of obscured AGNs which is thought to provide the bulk of the energy density in the X-ray background and possibly a significant fraction of the FIR background
Publication The XMM-Newton optical-UV monitor telescope . Mason, K. O., Breeveld, A., et all. . A&A . 365-36 . 2001 . 2001A&A...365L..36M ,
XMM-Newton observation of a distant X-ray selected cluster of galaxies at z=1.26 with possible cluster interaction . Hashimoto, Yasuhiro, Hasinger, Gunther, et all. . A&A . 381-841 . 2002 . 2002A&A...381..841H ,
XMM-Newton observation of the Lockman Hole. II. Spectral analysis . Mainieri, V., Bergeron, J., et all. . A&A . 393-425 . 2002 . 2002A&A...393..425M ,
An XMM-Newton study of the hard X-ray sky . Piconcelli, E., Cappi, M., et all. . A&A . 412-689 . 2003 . 2003A&A...412..689P ,
XMM-Newton observations of the Lockman Hole IV: spectra of the brightest AGN . Mateos, S., Barcons, X., et all. . A&A . 444-79 . 2005 . 2005A&A...444...79M ,
A revision of the X-ray absorption nature of BALQSOs . Streblyanska, A., Barcons, X., et all. . A&A . 515-2 . 2010 . 2010A&A...515A...2S ,
An X-ray-selected Galaxy Cluster in the Lockman Hole at Redshift 1.753 . Henry, J. Patrick, Salvato, Mara, et all. . ApJ . 725-615 . 2010 . 2010ApJ...725..615H ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
An Extremely Luminous Panchromatic Outburst ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-04-27T02:46:15Z/2000-05-19T19:46:53Z
Version PPS_NOT_AVAILABLE
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 2001-10-11T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2001-10-11T00:00:00Z, 012370, PPS_NOT_AVAILABLE. https://doi.org/10.5270/esa-s1pl1sx