A dataset provided by the European Space Agency

Name: XMM-Newton Observation toward the SNR candidate HESS J1912+101
Published: 2017-04-08T22:00:00Z

Proposal ID	076324
Title	XMM-Newton Observation toward the SNR candidate HESS J1912+101
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763240101
DOI	https://doi.org/10.5270/esa-zcrf4dy
Principal Investigator, PI	Dr Hidetoshi Sano
Abstract	HESS J1912+101 is one of the bright unidentified TeV sources discovered in theH.E.S.S. galactic plane survey. The source still has no clear counterpart anddeep observations in other wavelengths are desirable. Recently, HESS J1912+101is revealed to have a shell-like morphology similar to the supernova remnant RXJ1713.7-3946. If HESS J1912+101 is a SNR, we expect that relativistic particles(cosmic-ray protons and electrons) are accelerated efficiently in the object andare radiating synchrotron X-rays. Our aim is to detect synchrotron X-rays fromthis object for the first time, and estimate its nature. This observation andradio data will allow us to reveal the origin of the gamma-rays.
Publications	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	2016-03-18T09:29:55Z/2016-03-18T19:11:35Z
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	2017-04-08T22:00:00Z
Last Update	2025-01-27
Keywords	"galactic plane survey", "J1713.7", "hess j1912", "xmm newton", "gamma rays", "accelerated efficiently", "synchrotron xray", "XMM-Newton", "supernova remnant", "radiating synchrotron xray", "XMM", "HESS", "radio data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Hidetoshi Sano, 2017, 'XMM-Newton Observation toward the SNR candidate HESS J1912+101', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zcrf4dy