A dataset provided by the European Space Agency

Name: Completing the X-ray survey of HESS~J1614-518
Published: 2009-09-26T00:00:00Z

Proposal ID	055566
Title	Completing the X-ray survey of HESS~J1614-518
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555660101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555660201
DOI	https://doi.org/10.5270/esa-w5y9enh
Principal Investigator, PI	Prof Dieter Horns
Abstract	We propose to observe for the first time the south-eastern part of theunidentified very high energy E>100 GeV gamma-ray source HESS~J1614-518. In arecent XMM-Newton observation (36 ksec) of the north-eastern part of thissource, extended (FWHM ~8),non-thermal X-ray emission has been detected with anenergy flux $f(2-10)~1.5x10^{-12}cgs. The morphology of the X-ray emittingregion is similar to the morphology of HESS~J1614-518.With the proposedobservation of 40~ksec of the south-eastern part of HESS~J1614-518 which has sofar not beeen covered by X-ray observations, we want to search for X-rayemission from this region of HESS~J1614-518 which would clearly establish theclose connection between X-ray and VHE emission.
Publications	Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz Tobias \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P A search for new supernova remnant shells in the Galactic plane with H.E.S.S. \|H. E. S. S. Collaboration Abdalla H. et al. \| A&A \| 612-8 \| 2018 \| 2018A&A...612A...8H \| http://ui.adsabs.harvard.edu/#abs/2018A&A...612A...8H Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2008-08-15T02:10:53Z/2008-08-15T16:45:25Z
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	2009-09-26T00:00:00Z
Last Update	2025-01-27
Keywords	"5x10 ^{", "energy flux", "xray emitting region", "xmm newton", "XMM-Newton", "close connection", "beeen covered", "xray emission", "j1614 518", "XMM", "vhe emission", "HESS", "xray survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Dieter Horns, 2009, 'Completing the X-ray survey of HESS~J1614-518', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w5y9enh