A dataset provided by the European Space Agency

Name: Observing the cosmic-ray factory G335.2+0.1 - HESS J1626-490
Published: 2014-09-06T00:00:00Z

Proposal ID	072456
Title	Observing the cosmic-ray factory G335.2+0.1 - HESS J1626-490
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724560101
DOI	https://doi.org/10.5270/esa-5mqpvt6
Principal Investigator, PI	Dr Igor Telezhinsky
Abstract	We propose a 20-ksec observation of the Supernova Remnant G335.2+0.1. Theprincipal aim of the observation is to detect thermal radiation and use it toestablish the hydrodynamic parameters and evolutionary state of the remnant. Thesecondary aim is to detect possible non-thermal radiation to constrain themagnetic field at the shock and the efficiency of cosmic-ray acceleration in theobject. The dedicated textit{XMM-Newton} exposure of G335.2+0.1 would provide uswith vital X-ray data needed to understand the distribution of cosmic rays inthe system and the relation between G335.2+0.1 and the TeV-band source HESSJ1626-490 that is coincident with a nearby molecular cloud.
Publications	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	2013-08-14T00:35:00Z/2013-08-14T06:58:20Z
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	2014-09-06T00:00:00Z
Last Update	2025-01-27
Keywords	"thermal radiation", "vital xray data", "cosmic rays", "magnetic field", "xmm newton", "G335.2", "XMM-Newton", "hess j1626 490", "supernova remnant g335", "nearby molecular cloud", "nonthermal radiation", "dedicated textit", "XMM", "cosmic ray acceleration", "HESS", "hydrodynamic parameters"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Igor Telezhinsky, 2014, 'Observing the cosmic-ray factory G335.2+0.1 - HESS J1626-490', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5mqpvt6