A dataset provided by the European Space Agency

Name 031159
Title ToO and Discretionary Time
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311590901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311591001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311591101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0311591201
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DOI 10.5270/esa-8bryok6
Author Dr NORBERT SCHARTEL (PS)
Description Observation 1: RX J0720.4-3125, X-ray emitting, radio-quiet neutron star Observation 2: GRB 051103, possible short GRB or SGR in M81 ? Observation 3: Observation 4: V504 Cen - Cataclysmic variable Observation 5: XTE J1817-330, New Black Hole Candidate Observation 6: NOVA SMC 2005 Observation 7: Geminga Observation 8: GRB060218-SWIFTJ032139+165203 Observation 9: Swift J1753.5-0127 Observation 12: NOVA LMC 2005
Publication Evidence for precession of the isolated neutron star RX J0720.4-3125 . Haberl, F., Turolla, R., et all. . A&A . 451-17 . 2006 . 2006A&A...451L..17H ,
A self-consistent model of isolated neutron stars: the case of the X-ray pulsar RX J0720.4-3125 . Perez-Azorin, J. F., Pons, J. A., et all. . A&A . 459-175 . 2006 . 2006A&A...459..175P ,
XMM-Newton RGS spectrum of RX J0720.4-3125: an absorption feature at 0.57 keV . Hambaryan, V., Neuhauser, R., et all. . A&A . 497-9 . 2009 . 2009A&A...497L...9H ,
Discovery of a broad iron line in the black hole candidate Swift J1753.5-0127, and the disc emission in the low-hard state revisited . Hiemstra, Beike, Soleri, Paolo, et all. . MNRAS . 394-2080 . 2009 . 2009MNRAS.394.2080H ,
Determining the spin of two stellar-mass black holes from disc reflection signatures . Reis, R. C., Fabian, A. C., et all. . MNRAS . 395-1257 . 2009 . 2009MNRAS.395.1257R ,
Updated phase coherent timing solution of the isolated neutron star RX J0720.4-3125 using recent XMM-Newton and Chandra observations . Hohle, M. M., Haberl, F., et all. . A&A . 521-11 . 2010 . 2010A&A...521A..11H ,
New X-ray Observations of the Geminga Pulsar Wind Nebula . Pavlov, George G., Bhattacharyya, Sudip, . ApJ . 715-66 . 2010 . 2010ApJ...715...66P ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-11-12T06:02:45Z/2006-07-18T19:24:01Z
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 2006-10-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2006-10-06T00:00:00Z, 031159, 17.56_20190403_1200. https://doi.org/10.5270/esa-8bryok6