A dataset provided by the European Space Agency

Name 061000
Title Generic ToO-DDT Proposal for AO8
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0610000201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0610000301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0610000401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0610000501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0610000601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0610000701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0610000901

DOI 10.5270/esa-snvmp9y
Author Dr NORBERT SCHARTEL (PS)
Description obs 1: Cygnus X-1 in rev 1728. Non standard RGS readout sequence!!!!!!!! obs 2: PHL 1092 obs 6: SGR 0418+5729 obs 7: XTE J1652-453 obs 9: IGR J17511-3057
Publication Swift X-Ray Observations of Classical Novae. II. The Super Soft Source Sample . Schwarz, Greg J., Ness, Jan-Uwe, et all. . ApJS . 197-31 . 2011 . 2011ApJS..197...31S ,
Probing the Environment of Accreting Compact Objects . Hanke, Manfred, . PhDT . 0-9 . 2011 . 2011PhDT.........9H ,
The X-ray spectrum of the newly discovered accreting millisecond pulsar IGR J17511-3057 . Papitto, A., Riggio, A., et all. . MNRAS . 407-2575 . 2010 . 2010MNRAS.407.2575P ,
A strong and broad Fe line in the XMM-Newton spectrum of the new X-ray transient and black hole candidate XTE J1652-453 . Hiemstra, Beike, Mendez, Mariano, et all. . MNRAS . 411-137 . 2011 . 2011MNRAS.411..137H ,
Long-term spectral and timing properties of the soft gamma-ray repeater SGR 1833-0832 and detection of extended X-ray emission around the radio pulsar PSR B1830-08 . Esposito, P., Israel, G. L., et all. . MNRAS . 416-205 . 2011 . 2011MNRAS.416..205E ,
A magnetar strength surface magnetic field for the slowly spinning down SGR 0418+5729 . Guver, Tolga, Gogus, Ersin, . MNRAS . 418-2773 . 2011 . 2011MNRAS.418.2773G ,
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 . 423-35...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-05-06T10:14:15Z/2009-09-21T20:08:41Z
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 2010-04-13T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-04-13T00:00:00Z, 061000, 17.56_20190403_1200. https://doi.org/10.5270/esa-snvmp9y