A dataset provided by the European Space Agency

Name: Searching for the engine powering the TeV source MGRO J2019+37
Published: 2009-06-21T00:00:00Z

Proposal ID	055235
Title	Searching for the engine powering the TeV source MGRO J2019+37
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552350101
DOI	https://doi.org/10.5270/esa-4fs4llp
Principal Investigator, PI	Prof Josep Maria Paredes
Abstract	The MILAGRO Collaboration has recently reported the discovery of a new extendedand unidentified TeV source in the Cygnus region, MGRO J2019+37. Its location isconsistent with two EGRET sources, suggesting that it could be formed bymultiple unresolved sources. To find possible counterparts, we have conducted adeep radio survey discovering two jet-like sources which are positionallycoincident with each of the EGRET sources and with the inner box of MGROJ2019+37. One of them has morphological and spectral characteristics similar tothe microquasar 1E 1740.7-2942, the Great Annihilator at the Galactic Center. Wepropose to carry out a deep XMM-Newton observation covering the two radio jetsources to find their keV counterparts and constrain the mechanism responsible for the TeV 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 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	2008-05-08T09:58:14Z/2008-05-09T04:24:20Z
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	2009-06-21T00:00:00Z
Keywords	"deep xmm newton", "unidentified tev source", "multiple unresolved sources", "XMM", "spectral characteristics", "microquasar 1e 1740", "tev emission", "egret sources", "inner box", "engine powering", "mgro j2019", "galactic center", "radio jet sources", "XMM-Newton", "kev counterparts", "positionally coincident", "cygnus region", "milagro collaboration"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Josep Maria Paredes, 2009, 'Searching for the engine powering the TeV source MGRO J2019+37', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4fs4llp