A dataset provided by the European Space Agency

Name: Searching for the first radio-quiet'' gamma-ray emitting millisecond pulsar
Published: 2015-01-14T23:00:00Z

Proposal ID	072113
Title	Searching for the first radio-quiet gamma-ray emitting millisecond pulsar
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721130101
DOI	https://doi.org/10.5270/esa-a3i0oly
Principal Investigator, PI	Prof Albert Kong
Abstract	We propose to observe a gamma-ray millisecond pulsar (MSP) candidate, 2FGLJ2339.6-0532, to search for the first radio-quiet gamma-ray emitting MSP ina binary. The Fermi source has a candidate X-ray counterpart from Chandra dataand its X-ray and gamma-ray properties are consistent with known gamma-raypulsars. The source is also found to have a 4.53-hr orbital period in X-ray andoptical data. We propose to use the timing mode of XMM-Newton to search formillisecond pulsation. Moreover, the high quality energy spectra will allow usto study the spectral properties and phase resolved spectra to constrain thesystem geometry.
Publications	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 A Gaia view of the optical and X-ray luminosities of compact binary millisecond pulsars \|Koljonen Karri I. I. Linares Manuel \| MNRAS \| 525-3963 \| 2023 \| 2023MNRAS.525.3963K \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.525.3963K Modeling X-Ray and Gamma-Ray Emission from Redback Pulsar Binaries \|Sim Minju An Hongjun \| ApJ \| 964-109 \| 2024 \| 2024ApJ...964..109S \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...964..109S 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 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	2013-12-14T23:14:26Z/2013-12-15T17:01:05Z
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	2015-01-14T23:00:00Z
Last Update	2025-01-27
Keywords	"quality energy spectra", "optical data", "chandra data", "J2339.6", "gamma ray properties", "xmm newton", "millisecond pulsation", "2fgl j2339", "XMM-Newton", "gamma ray pulsars", "spectral properties", "system geometry", "hr orbital period", "XMM", "fermi source", "phase resolved spectra", "candidate xray counterpart"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Albert Kong, 2015, 'Searching for the first radio-quiet'' gamma-ray emitting millisecond pulsar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-a3i0oly