A dataset provided by the European Space Agency

Name: Pulse Searches of Probable GeV Pulsars Associated with TeV Sources
Published: 2010-03-31T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	055570
Title	Pulse Searches of Probable GeV Pulsars Associated with TeV Sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555700101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555700201
DOI	https://doi.org/10.5270/esa-n7vyfuo
Principal Investigator, PI	Dr Mallory Roberts
Abstract	There are several likely pulsars in EGRET error boxes which have been detectedin X-rays and are probably associated with known TeV sources. Here we proposeXMM-Newton studies of three of them: GeV J1825-1310 (the Eel), the Rabbit, andGeV J1907+0557, with the primary goal of detecting pulsations using the PN insmall window mode. They are also within X-ray pulsar wind nebulae, and the MOSimagers will be useful in studying the large scale structure of the nebulae.
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 soft gamma-ray pulsar population: a high-energy overview \|Kuiper L. Hermsen W. \| MNRAS \| 449-3827 \| 2015 \| 2015MNRAS.449.3827K \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.3827K 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 Characterizing X-Ray Properties of the Gamma-Ray Pulsar PSR J1418-6058 in the Rabbit Pulsar Wind Nebula \|Kim Minjun An Hongjun \| ApJ \| 892-5 \| 2020 \| 2020ApJ...892....5K \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892....5K The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars \|Papitto A. Falanga M. et al. \| NewAR \| 91-101544 \| 2020 \| 2020NewAR..9101544P \| http://ui.adsabs.harvard.edu/#abs/2020NewAR..9101544P 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 A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058 \|Park Jaegeun Kim Chanho et al. \| ApJ \| 945-66 \| 2023 \| 2023ApJ...945...66P \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...945...66P 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2009-02-21T14:13:00Z/2009-02-23T03:39:40Z
Version	PPS_NOT_AVAILABLE
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	2010-03-31T00:00:00Z
Last Update	2026-07-09
Keywords	"pulse searches", "XMM-Newton", "gev j1907", "scale structure", "probable gev pulsars", "gev j1825 1310", "mos imagers", "tev sources", "XMM", "egret error boxes", "window mode", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mallory Roberts, 2010, 'Pulse Searches of Probable GeV Pulsars Associated with TeV Sources', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-n7vyfuo
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.