A dataset provided by the European Space Agency

Proposal ID 060547
Title XMM-Newton Observations of Unidentified High Latitude Fermi Sources
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DOI https://doi.org/10.5270/esa-zceyabc
Principal Investigator, PI Dr Michael Wolff
Abstract We propose to observe with XMM-Newton a selected set of 7 Fermi-LAT observedhigh galactic latitude gamma-ray sources that as yet have no identifiedcounterparts in any other energy range. These sources have been detected by theFermi-LAT with high confidence and are either active galactic nuclei, galacticpulsars, or an as-yet unidentified new class of gamma-ray sources. The proposedobservations are for 20 ks per source covering the Fermi-LAT source errorregion. We will determine the X-ray flux for any sources detected by XMM-Newtonwithin the Fermi-LAT region, and characterize the source spectra and temporalproperties in the 0.2-10 keV energy band for these sources. A parallel proposalhas been submitted to the VLA to map the same Fermi-LAT source regions.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-07-15T08:05:59Z/2010-04-21T19:21:29Z
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 2011-05-15T00:00:00Z
Keywords "galactic pulsars", "temporal properties", "latitude fermi sources", "fermi lat", "XMM", "xmm newton", "xray flux", "energy range", "source spectra", "active galactic nuclei", "kev energy band", "XMM-Newton", "fermi lat region", "gamma ray sources"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Michael Wolff, 2011, 'XMM-Newton Observations of Unidentified High Latitude Fermi Sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zceyabc