A dataset provided by the European Space Agency

Name: The composite unidentified source HESS J1843-033
Published: 2011-10-29T00:00:00Z

Proposal ID	065496
Title	The composite unidentified source HESS J1843-033
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0654960101
DOI	https://doi.org/10.5270/esa-xzn3se8
Principal Investigator, PI	Dr Omar Tibolla
Abstract	In a survey of the Galactic plane performed in 2007 with the High EnergyStereoscopic System (H.E.S.S.) many new sources have been discovered and most ofthem are still unidentified. We propose to use XMM-Newton to perform follow-upobservations on one of the brightest newly discovered sources, HESS J1843-033,to identify its possible X-ray counterparts. An offset PWN is one of thepossible explanations for HESS J1843-033, but this hypothesis is still underinvestigation. The aim is to obtain the morphological and spectral informationof the possible counterparts in helping to understand the emission mechanism ofthis source.
Publications	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	2010-09-24T22:49:05Z/2010-09-25T07:41:04Z
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	2011-10-29T00:00:00Z
Last Update	2025-01-27
Keywords	"galactic plane performed", "hess j1843 033", "xmm newton", "offset pwn", "XMM-Newton", "emission mechanism", "energy stereoscopic system", "spectral information", "XMM", "HESS", "xray counterparts"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Omar Tibolla, 2011, 'The composite unidentified source HESS J1843-033', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xzn3se8