A dataset provided by the European Space Agency

Name 065820
Title Planck Clusters Follow up II (DDT)
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658200101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658200201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658200301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658200401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658200501
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658200801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658200901
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658201001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658201101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658201201
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0658201301

DOI 10.5270/esa-aro6d01
Author Dr Norbert Schartel (DDT)
Description Follow-up of Planck Clusters (cont)
Publication Planck early results. XXVI. Detection with Planck and confirmation by XMM-Newton of PLCK G266.6-27.3, an exceptionally X-ray luminous and massive galaxy cluster at z ~ 1 . Planck Collaboration, Aghanim, N., et all. . A&A . 536-26 . 2011 . 2011A&A...536A..26P ,
Planck intermediate results. I. Further validation of new Planck clusters with XMM-Newton . Planck Collaboration, Aghanim, N., et all. . A&A . 543-102 . 2012 . 2012A&A...543A.102P ,
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 ,
Baryon content of massive galaxy clusters at 0.57 < z < 1.33 . Chiu, I., Mohr, J., et all. . MNRAS . 455-258 . 2016 . 2016MNRAS.455..258C ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 . Pons, E., Watson, M. G., . A&A . 594-72 . 2016 . 2016A&A...594A..72P ,
Dependence of the broad Fe Kalpha line on the physical parameters of AGN . Liu, Zhu, Yuan, Weimin, et all. . MNRAS . 463-684 . 2016 . 2016MNRAS.463..684L ,
Resolving gal...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-12-22T08:29:35Z/2011-05-16T20:52:23Z
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 2011-12-25T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-12-25T00:00:00Z, 065820, 17.56_20190403_1200. https://doi.org/10.5270/esa-aro6d01