A dataset provided by the European Space Agency

Name: Search for X-ray counterparts of radio-quiet MSPs in Fermi LAT sources
Published: 2013-09-06T00:00:00Z

Proposal ID	069283
Title	Search for X-ray counterparts of radio-quiet MSPs in Fermi LAT sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692830101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692830201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0692830301
DOI	https://doi.org/10.5270/esa-7fjrcuj
Principal Investigator, PI	Dr Pablo Saz Parkinson
Abstract	The Large Area Telescope (LAT) on Fermi has detected ~100 gamma-ray pulsars andrevolutionized our understanding of these objects and their high-energyemission. One important open question is whether there are any radio-quietgamma-ray MSPs. The answer has profound implications for our understanding ofthe geometry and emission mechanisms of pulsars. Blind searches for gamma-rayMSPs are hampered by the large uncertainties in LAT positions. We propose to useXMM to identify plausible X-ray counterparts of 4 bright high-Galactic-latitudeLAT sources which are plausible radio-quiet MSP. This will enable sensitiveblind searches for pulsations in LAT data. We will determine the X-ray position,flux, and spectral properties in the 0.3-10 keV energy band for any X-ray sources detected.
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 X-ray observations and the search for Fermi-LAT gamma-ray pulsars \|Saz Parkinson P. M. Belfiore A. et al. \| AN \| 335-291 \| 2014 \| 2014AN....335..291S \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..291S On the origin of two unidentified radio/X-ray sources discovered with XMM-Newton \|Garcia Federico Combi Jorge A. et al. \| A&A \| 584-65 \| 2015 \| 2015A&A...584A..65G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...584A..65G Searches for Millisecond Pulsar Candidates among the Unidentified Fermi Objects \|Hui C. Y. Park S. M. et al. \| ApJ \| 809-68 \| 2015 \| 2015ApJ...809...68H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...809...68H Classification and Ranking of Fermi LAT Gamma-ray Sources from the 3FGL Catalog using Machine Learning Techniques \|Saz Parkinson P. M. Xu H. et al. \| ApJ \| 820-8 \| 2016 \| 2016ApJ...820....8S \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...820....8S 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 A multiwavelength investigation of candidate millisecond pulsars in unassociated gamma-ray sources \|Salvetti D. Mignani R. P. et al. \| MNRAS \| 470-466 \| 2017 \| 2017MNRAS.470..466S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..466S Identification of candidate millisecond pulsars from Fermi LAT observations II \|Dai Xue-Jie Wang Zhong-Xiang et al. \| RAA \| 17-72 \| 2017 \| 2017RAA....17...72D \| http://ui.adsabs.harvard.edu/#abs/2017RAA....17...72D Astrofisica de altas energias de objetos compactos \|Combi J. A. \| BAAA \| 57-209 \| 2015 \| 2015BAAA...57..209C \| http://ui.adsabs.harvard.edu/#abs/2015BAAA...57..209C Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar \|Clark Colin J. Pletsch Holger J. et al. \| SciA \| 4-7228 \| 2018 \| 2018SciA....4.7228C \| http://ui.adsabs.harvard.edu/#abs/2018SciA....4.7228C 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-06-16T12:17:48Z/2012-08-21T10:25:14Z
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	2013-09-06T00:00:00Z
Last Update	2025-01-27
Keywords	"kev energy band", "lat data", "radio quiet msps", "emission mechanisms", "radio quiet msp", "lat positions", "xray position", "gamma ray pulsars", "profound implications", "xray counterparts", "sensitive blind searches", "telescope lat", "blind searches", "gamma ray msps", "spectral properties", "xray sources", "fermi lat sources", "energy emission", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Pablo Saz Parkinson, 2013, 'Search for X-ray counterparts of radio-quiet MSPs in Fermi LAT sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-7fjrcuj