A dataset provided by the European Space Agency

Name: The two brightest unidentified Galactic sources of the new H.E.S.S. survey
Published: 2010-03-07T00:00:00Z

Proposal ID	055631
Title	The two brightest unidentified Galactic sources of the new H.E.S.S. survey
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556310201
DOI	https://doi.org/10.5270/esa-mk3mtv6
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.) a lot of new sources have been discovered andmost of them are still unidentified. We propose to use XMM-Newton to performfollow-up on the two brightest newly discovered sources, namely HESS J1507-622and HESS J1843-033, to identify their possible X-ray counterparts. Both sourceshave no clear positional counterparts: HESS J1507-622 does not show anycounterpart at all, whereas an offset PWN is one of the possible explanationsfor HESS J1843-033. The aim is to obtain the morphological and spectralinformation of the possible counterpart in helping to understand the emissionmechanism of these 2 sources: the predicted X-ray flux is sufficient for detailed studies of these sources.
Publications	XMM-Newton and Chandra X-ray follow-up observations of the VHE gamma-ray source HESS J1507-622 \|Tibolla, O., Kaufmann, S., \| A&A \| 567-74 \| 2014 \| 2014A&A...567A..74T \| http://ui.adsabs.harvard.edu/#abs/2014A&A...567A..74T 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 Exploring the potential X-ray counterpart of the puzzling TeV gamma-ray source HESS J1507-622 with new Suzaku observations \|Eger, P., Domainko, W. F., \| MNRAS \| 447-3564 \| 2015 \| 2015MNRAS.447.3564E \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447.3564E 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 Discovery and follow-up studies of the extended, off-plane, VHE gamma-ray source HESS J1507-622 \|H.E.S.S. Collaboration, Acero, F., et al. \| A&A \| 525-45 \| 2011 \| 2011A&A...525A..45H \| http://ui.adsabs.harvard.edu/#abs/2011A&A...525A..45H 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	2009-01-27T20:52:24Z/2009-01-28T04:35:27Z
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	2010-03-07T00:00:00Z
Keywords	"galactic plane performed", "XMM", "emission mechanism", "predicted xray flux", "offset pwn", "energy stereoscopic system", "HESS", "hess j1843 033", "xray counterparts", "XMM-Newton", "positional counterparts", "spectral information", "hess j1507 622", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Omar Tibolla, 2010, 'The two brightest unidentified Galactic sources of the new H.E.S.S. survey', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mk3mtv6