A dataset provided by the European Space Agency

Name 081088
Title EPIC Gain, contamination and CTI monitoring-1ES0102
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810880901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810881001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810881301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810881401
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0810881501

DOI https://doi.org/10.5270/esa-xpsoxpp
Author European Space Agency
Description EPIC ROUTINE CAL - The AXAF standard candle source, 1ES0102-72 in the SMC region
will be observed periodically. The strong emission lines at low energies will be
measured to determine the CCD gain and CTI at the boresight location.
In addition, apparent secular changes in various emission line strengths
may be used to track contamination build-up.
(was proposal 13572)
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2018-10-28T11:30:42Z/2023-10-26T16:38:50Z
Version 20.10_20230417_1156
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 2023-11-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2023, Epic Gain Comma Contamination And Cti Monitoring-1Es0102, 20.10_20230417_1156, European Space Agency, https://doi.org/10.5270/esa-xpsoxpp