A dataset provided by the European Space Agency

Name: XMM-Newton observations of Fermi detected pulsars
Published: 2012-03-26T00:00:00Z

Proposal ID	065502
Title	XMM-Newton observations of Fermi detected pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655020101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655020201
DOI	https://doi.org/10.5270/esa-vs7i0uf
Principal Investigator, PI	Dr Natalie Webb
Abstract	We propose to make XMM-Newton observations of six pulsars detected with theFermi LAT to increase the number of pulsars for which good X-ray, gamma-ray andradio data exist in order to constrain the mechanism which generates the pulsarhigh energy emission. For four of the proposed pulsars this will be the firstobservation in X-rays. We will use both the spectra and phase-folded lightcurvesto discriminate between differing models for the high energy emission such asthe polar cap, slot gap or outer gap models. XMM-Newton is the only observatorywith sufficient collecting area and high enough timing resolution to detectthese pulsars and to obtain the spectra and lightcurves, necessary todiscriminate between the high energy models.
Publications	X-ray follow-up observations of the two gamma-ray pulsars PSR J1459-6053 and PSR J1614-2230 \|Pancrazi B. Webb N. A. et al. \| A&A \| 544-108 \| 2012 \| 2012A&A...544A.108P \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A.108P 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 Case for PSR J1614--2230 as a NICER Target \|Miller M. Coleman \| ApJ \| 822-27 \| 2016 \| 2016ApJ...822...27M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...27M 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 NICER X-Ray Observations of Seven Nearby Rotation-powered Millisecond Pulsars \|Guillot Sebastien Kerr Matthew et al. \| ApJ \| 887-27 \| 2019 \| 2019ApJ...887L..27G \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887L..27G Multiwavelength constraints on the unidentified Galactic TeV sources HESS J1427-608 HESS J1458-608 and new VHE u03b3-ray source candidates \|Devin J. Renaud M. et al. \| A&A \| 647-68 \| 2021 \| 2021A&A...647A..68D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...647A..68D 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2011-02-12T06:23:38Z/2011-03-01T01:11:04Z
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	2012-03-26T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "gamma ray", "XMM-Newton", "radio data exist", "energy emission", "outer gap models", "slot gap", "xmm newton", "phase folded lightcurves", "fermi lat", "polar cap", "energy models", "differing models"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Natalie Webb, 2012, 'XMM-Newton observations of Fermi detected pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vs7i0uf