A dataset provided by the European Space Agency

Name 009501
Title In-orbit measurement of the XMM telescope vignetting function
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095010901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0095011501

DOI 10.5270/esa-376kiza
Author Dr Fred Jansen XMM-Newton PS
Description CAL- Observations of the compact cluster of galaxies A496 at different off-axis angles will provide changes in count rates for different energy bands. These will be used to derive the vignetting function of the XMM telescopes in different energy bands.
Publication XMM-Newton observations of the cluster of galaxies Abell 496. Measurements of the elemental abundances in the intracluster medium . Tamura, T., Bleeker, J. A. M., et all. . A&A . 379-107 . 2001 . 2001A&A...379..107T ,
Cold fronts in galaxy clusters . Ghizzardi, S., Rossetti, M., . A&A . 516-32 . 2010 . 2010A&A...516A..32G ,
The cool-core bias in X-ray galaxy cluster samples. I. Method and application to HIFLUGCS . Eckert, D., Molendi, S., . A&A . 526-79 . 2011 . 2011A&A...526A..79E ,
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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
X-Ray Morphological Analysis of the Planck ESZ Clusters . Lovisari, Lorenzo, Forman, William R., et all. . ApJ . 846-51 . 2017 . 2017ApJ...846...51L ,
Charge exchange in galaxy clusters . Gu, Liyi, Mao, Junjie, et all. . A&A . 611-26 . 2018 . 2018A&A...611A..26G ,
X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton . Lovisari, Lorenzo, Schellenberger, Gerrit, et all. . ApJ . 892-102 . 2020 . 2020ApJ...892..102L ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-03-13T10:00:29Z/2000-03-15T01:31:26Z
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 2000-03-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2000-03-09T00:00:00Z, 009501, 17.56_20190403_1200. https://doi.org/10.5270/esa-376kiza