A dataset provided by the European Space Agency

Name 013472
Title Capella: RGS wavelength scale calibration
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134720101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134720401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134720801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134720901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134721001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134721101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134721201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134721501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134721601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134721701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134722001
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134722101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0134722201

DOI https://doi.org/10.5270/esa-tf0cisa
Author Dr Fred Jansen XMM-Newton PS
Description Routine Calibration - RGS wavelength scale

obs2 is the standard setup with EPIC closed ff and should be copied for
scheduling. OM blocked to be replaced by internal calibration observations
according to recipe.
Obs#13 and #14 for rev. ca. 868 (Chandra coord)
Obs#16 and #17 for Chandra coord obs March 28 2005
Obs#20 for Chandra coord March 2006
Obs#21 for XCAL Feb-March 2007
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-03-15T19:19:40Z/2007-02-21T10:53:40Z
Version PPS_NOT_AVAILABLE
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 2007-02-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Fred Jansen XMM-Newton PS, 2007, 013472, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-tf0cisa