A dataset provided by the European Space Agency

Proposal ID 050567
Title Monitoring Sgr A* X-ray flaring activity to measure quasi periodic modulation
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505670101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505670201

DOI https://doi.org/10.5270/esa-5jvaylv
Principal Investigator, PI Dr Andrea Goldwurm
Abstract Building on the great successes of the monitoring program of Sgr A* flaringactivity we initiated and fostered in the last years, we propose to continueextended observations of the Galactic nucleus with XMM-Newton in order tofurther test the supermassive black hole paradigm while studying the accretionflow and radiation mechanisms associated with this unique system at the centreof the Galaxy. Thanks to the unique capabilities of XMM-Newton we will tacklecrucial questions that remain unanswered: 1) are X-ray flares from Sgr A* causedby blobs of hot, orbiting plasma in the accretion flow close to the eventhorizon of the black hole,
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-03-23T12:57:54Z/2008-03-24T20:20:48Z
Version 17.56_20190403_1200
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 2009-04-15T00:00:00Z
Keywords "orbiting plasma", "XMM", "galactic nucleus", "quasi periodic modulation", "xray flaring activity", "accretion flow close", "flaring activity", "xray flare", "event horizon", "black hole", "supermassive blackhole paradigm", "XMM-Newton", "accretion flow", "radiation mechanisms", "xmm newton"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Andrea Goldwurm, 2009, 'Monitoring Sgr A* X-ray flaring activity to measure quasi periodic modulation', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5jvaylv