A dataset provided by the European Space Agency

Name: Pulse Searches of Two Radio Quiet GeV Pulsars Associated with TeV Sources
Published: 2011-05-20T00:00:00Z

Proposal ID	060570
Title	Pulse Searches of Two Radio Quiet GeV Pulsars Associated with TeV Sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605700201
DOI	https://doi.org/10.5270/esa-xzmgo24
Principal Investigator, PI	Dr Mallory Roberts
Abstract	There are several likely gamma-ray pulsars in EGRET error boxes which areprobably associated with known TeV sources, but radio searches have failed todetect pulsations from them. Direct searches for gamma-ray pulsations of thebrightest EGRET sources using Fermi are proving quite successful. However, tounderstand the emission mechanisms, pulsations at other wavelengths arecritical. Here we propose XMM-Newton studies of two such sources: GeV J1825-1310(the Eel) and GeV J1907+0557, with the primary goal of detecting X-raypulsations using the PN in small window mode. Both have extended X-ray nebulawhose spatial and spectral properties will be studied using the MOS imagers.
Publications	The Second Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars \|Abdo A. A. Ajello M. et al. \| ApJS \| 208-17 \| 2013 \| 2013ApJS..208...17A \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..208...17A 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 Investigating the Nature of MGRO J1908+06 with Multiwavelength Observations \|Li Jian Liu Ruo-Yu et al. \| ApJ \| 913-33 \| 2021 \| 2021ApJ...913L..33L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...913L..33L Multiwavelength investigation of the candidate Galactic PeVatron MGRO J1908+06 \|Crestan S. Giuliani A. et al. \| MNRAS \| 505-2309 \| 2021 \| 2021MNRAS.505.2309C \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.2309C Exploring the Hadronic Origin of LHAASO J1908+0621 \|De Sarkar Agnibha Gupta Nayantara \| ApJ \| 934-118 \| 2022 \| 2022ApJ...934..118D \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...934..118D Investigating the radiative properties of LHAASO J1908 + 0621 \|Wu Keyao Zhou Liancheng et al. \| MNRAS \| 519-1881 \| 2023 \| 2023MNRAS.519.1881W \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.1881W Determining the Origin of Very-high-energy Gamma Rays from Galactic Sources by Future Neutrino Observations \|Song Bo-Heng Huang Tian-Qi \| ApJ \| 961-254 \| 2024 \| 2024ApJ...961..254S \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..254S 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	2010-04-26T09:32:55Z/2010-04-27T00:09:00Z
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	2011-05-20T00:00:00Z
Last Update	2025-01-27
Keywords	"mos imagers", "gamma ray pulsations", "radio searches", "egret error boxes", "xray nebula", "xmm newton", "window mode", "brightest egret sources", "XMM-Newton", "gamma ray pulsars", "gev j1907", "tev sources", "spectral properties", "xray pulsations", "pulse searches", "XMM", "gev j1825 1310", "emission mechanisms"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mallory Roberts, 2011, 'Pulse Searches of Two Radio Quiet GeV Pulsars Associated with TeV Sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xzmgo24