A dataset provided by the European Space Agency

Name: Measurement of the Al thickness of RGS2 CCD2
Published: 2000-12-05T00:00:00Z

Proposal ID	013272
Title	Measurement of the Al thickness of RGS2 CCD2
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0132721201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0132721301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0132721401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0132721501
DOI	https://doi.org/10.5270/esa-juvftzu
Principal Investigator, PI	Dr Fred Jansen XMM-Newton PS
Abstract	RGS2 CCD2 shows lower QE, although the gain and the redistribution look ok.- test hypothesis that Al filter-layer is thicker than specified.(NCRObs requested by C. Erd)
Publications	Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2000-12-03T15:10:56Z/2000-12-04T02:16:40Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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	2000-12-05T00:00:00Z
Keywords	"rgs2 ccd2", "lower qe", "ncrobs requested", "test hypothesis", "al filter layer", "al thickness", "redistribution look ok"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen XMM-Newton PS, 2000, 'Measurement of the Al thickness of RGS2 CCD2', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-juvftzu