A dataset provided by the European Space Agency

Name 051100
Title Monitoring observations of the Galactic Center region
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511000901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511001001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511001101
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511001201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511001301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0511001401

DOI https://doi.org/10.5270/esa-kvda05f
Author European Space Agency
Description We propose to continue our Chandra and XMM-Newton monitoring campaign of the 1.2
square degree region centered on Sgr A*. We will be able to detect very faint
transients with a peak luminosity of 1E33-1E35 ergs/s, 10-1000 times more
sensitive than would be possible with other satellites. This allows us to
observe a poorly studied group of transients and to follow the luminosity
behavior of faint (1E34-1E36 ergs/s) persistent sources. The Chandra
observations are necessary to facilitate rapid follow-up observations of the
detected transients at IR and radio wavelengths; the XMM-Newton observations are
needed to increase the likelihood of detecting transients in outburst and to
obtain better constraints on the long-term time averaged accretion rates of the transients present in the FOV.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-03-03T20:20:56Z/2008-09-27T15:53:26Z
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 2009-11-14T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009, Monitoring Observations Of The Galactic Center Region, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kvda05f