A dataset provided by the European Space Agency

Name 041299
Title EPIC Gain, contamination and CTI monitoring-Vela SNR
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412990901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991301
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0412991601

DOI https://doi.org/10.5270/esa-cttuza4
Author Dr Fred Jansen XMM-Newton MM
Description EPIC Routine Calibration: spectral capabilities and contamination monitoring PA=102 shall be used as default (was proposal 015976). obs1: exceptionally pointed at RA 08:49:30.0 Dec -45:35:00 (req. by K. Dennerl) (normally at RA 08:48:49.05 Dec -45:38:26.1) obs6: coord. changed to RA 08:48:49 Dec -45:38:27 (req. by K. Dennerl)
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-11-09T00:38:22Z/2017-10-31T09:44:04Z
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 2017-11-06T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-11-06T23:00:00Z, 041299, 17.56_20190403_1200. https://doi.org/10.5270/esa-cttuza4