A dataset provided by the European Space Agency

Name: Are HESS J1849-000 and HESS J1626-490 Powered by PulsarsquestionMark
Published: 2012-04-06T00:00:00Z

Proposal ID	065193
Title	Are HESS J1849-000 and HESS J1626-490 Powered by Pulsars?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651930201
DOI	https://doi.org/10.5270/esa-brd8wmf
Principal Investigator, PI	Dr Regis Terrier
Abstract	Detecting the pulsars that power Galactic TeV sources is the key tounderstanding the origin of those that remain unidentified. We have twoexcellent new X-ray candidates to search for pulsations, from XMM observationsof the Integral source IGR J18490-0000 coincident with the compact TeV sourceHESS J1849-000, and XMMU J162703.03-491232.7 found within the TeV extent of HESSJ1626-490. Both are bright, non-thermal point sources with a faint nebula. Allcharacteristics of these objects resemble those of young, energetic pulsars.Finding the expected pulsations will allow us to determine their energetics,critical for understanding the luminosity and size of their TeV nebulae.
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 Ancient Pulsar Wind Nebulae as a natural explanation for unidentified gamma-ray sources \|Kaufmann, S., Tibolla, O., \| NPPP \| 297-91 \| 2018 \| 2018NPPP..297...91K \| http://ui.adsabs.harvard.edu/#abs/2018NPPP..297...91K Studies of high-energy pulsars: The special case of PSR J1849-0001 \|Vleeschower Calas, Laila, Kaufmann, Sarah, et al. \| NPPP \| 297-102 \| 2018 \| 2018NPPP..297..102V \| http://ui.adsabs.harvard.edu/#abs/2018NPPP..297..102V 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 X-Ray Characterization of the Pulsar PSR J1849-0001 and Its Wind Nebula G32.64+0.53 Associated with TeV Sources Detected by H.E.S.S., HAWC, Tibet AS\\u03b3, and LHAASO \|Kim, Chanho, Park, Jaegeun, et al. \| ApJ \| 960-78 \| 2024 \| 2024ApJ...960...78K \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...960...78K Efficiency of Nonthermal Pulsed Emission from Eight MeV Pulsars \|Takata, J., Wang, H. -H., et al. \| ApJ \| 965-126 \| 2024 \| 2024ApJ...965..126T \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...965..126T 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	2011-03-23T22:53:58Z/2011-03-24T13:47:33Z
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	2012-04-06T00:00:00Z
Keywords	"03 491232", "hess j1849 000", "hess j1626 490", "XMM", "tev extent", "faint nebula", "xray candidates", "objects resemble", "tev nebulae", "HESS", "energetic pulsars", "pulsars ?.", "xmmu j162703"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Regis Terrier, 2012, 'Are HESS J1849-000 and HESS J1626-490 Powered by PulsarsquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-brd8wmf