A dataset provided by the European Space Agency

Name 051118
Title EPIC Routine Calibration: Tycho SNR
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511180101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511180201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511180301

DOI 10.5270/esa-6pz48mc
Author Dr Arvind Parmar XMM-Newton MM
Description EPIC Non Routine Calibration (NRCO#71): Tycho SNR CTE Calibration using CAL source and SNR PA fixed to 45 degr (i.e. to be scheduled in August) (if not possible, PA=225) (original proposal was 31059 - PI F. Jansen)
Publication An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L ,
Automatic Classification of Time-variable X-Ray Sources . Lo, Kitty K., Farrell, Sean, et all. . ApJ . 786-20 . 2014 . 2014ApJ...786...20L ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Discovery of a 3.5 keV line in the Galactic Centre and a critical look at the origin of the line across astronomical targets . Jeltema, Tesla, Profumo, Stefano, . MNRAS . 450-2143 . 2015 . 2015MNRAS.450.2143J ,
Spatial Distribution of X-Ray Emitting Ejecta in Tycho.s SNR: Indications of Shocked Titanium . Miceli, M., Sciortino, S., et all. . ApJ . 805-120 . 2015 . 2015ApJ...805..120M ,
Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus . ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-12-30T19:32:51Z/2008-01-03T08:12:15Z
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 2008-01-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-01-04T00:00:00Z, 051118, 17.56_20190403_1200. https://doi.org/10.5270/esa-6pz48mc