A dataset provided by the European Space Agency

Name: EPIC GAIN, CTE AND CONTAMINATION MONITORING-N132D
Published: 2024-02-23T00:00:00Z

Proposal ID	081101
Title	EPIC GAIN, CTE AND CONTAMINATION MONITORING-N132D
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811012401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811012501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811012601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811012701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811012801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811013001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811013101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811013201
DOI	https://doi.org/10.5270/esa-mdcb0e2
Principal Investigator, PI	Dr Peter Kretschmar XMM-Newton MM
Abstract	Routine CAL - During periods of low visibility, the primary target 1es0102 willbe supplemented by observations of the bright LMC supernova remnant N132D. Normally pn shall be in sw mode.Coords and PA constraints as in last obs (was 41418/09).
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 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	2018-02-23T06:04:21Z/2024-02-15T13:39:48Z
Version	PPS_NOT_AVAILABLE
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	2024-02-23T00:00:00Z
Last Update	2025-01-27
Keywords	"EPIC", "routine cal", "low visibility", "sw mode", "epic gain", "pa constraints", "primary target 1es0102"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Peter Kretschmar XMM-Newton MM, 2024, 'EPIC GAIN, CTE AND CONTAMINATION MONITORING-N132D', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-mdcb0e2