A dataset provided by the European Space Agency

Name: The first Fermi pulsar with an X-ray spectral feature
Published: 2017-04-14T22:00:00Z

Proposal ID	076402
Title	The first Fermi pulsar with an X-ray spectral feature
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764020101
DOI	https://doi.org/10.5270/esa-ohmq8qr
Principal Investigator, PI	Dr Andrey Danilenko
Abstract	Analysis of the first 20-ks Chandra observation of the bright radio-quiet Fermipulsar J0633+0632 reveals an absorption feature in its spectrum near 0.8 keV.Besides that, it is likely the coldest neutron star at the neutrino coolingstage. However, a low number of source counts in Chandra data does not allow toconstrain the line shape and the thermal continuum origin. We propose deepobservations with XMM-Newton to establish the absorption feature shape, toexplore the continuum, and to search for X-ray pulsations with the pulsarperiod.
Publications	Spectral characterization of the non-thermal X-ray emission of gamma-ray pulsars \|Coti Zelati Francesco Torres Diego F. et al. \| MNRAS \| 492-1025 \| 2020 \| 2020MNRAS.492.1025C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.492.1025C XMM-Newton observations of a gamma-ray pulsar J0633+0632: pulsations cooling and large-scale emission \|Danilenko A. Karpova A. et al. \| MNRAS \| 493-1874 \| 2020 \| 2020MNRAS.493.1874D \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.1874D 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 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	2016-03-31T05:32:14Z/2016-04-01T07:22:14Z
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	2017-04-14T22:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "0632 reveals", "XMM-Newton", "neutrino cooling stage", "xray pulsations", "line shape", "chandra data", "xmm newton", "xray spectral", "fermi pulsar", "source counts", "thermal continuum origin", "coldest neutron star", "pulsar period"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andrey Danilenko, 2017, 'The first Fermi pulsar with an X-ray spectral feature', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ohmq8qr