A dataset provided by the European Space Agency

Name: Young, hot PSR J1357-6429 and its PWN
Published: 2010-09-02T00:00:00Z

Proposal ID	060328
Title	Young, hot PSR J1357-6429 and its PWN
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0603280101
DOI	https://doi.org/10.5270/esa-9b1wps0
Principal Investigator, PI	Dr George Pavlov
Abstract	Observations of thermal components in the X-ray spectra of young pulsars provideinsights into fundamental physics of neutron star interiors and magnetospheres.A short XMM-Newton exposure of the 7 kyr old PSR J1357 6429 has revealed thermalemission from the NS surface and an elongated diffuse feature extending from thepulsar, most likely a pulsar wind nebula (PWN). Observations with Chandra HRC-Shave have provided tentative detections of a compact PWN and pulsations. Here wepropose a detailed study of the pulsars spectral and timing properties, anddeep imaging and spectroscopy of the PWN with XMM-Newton and Chandra.
Publications	X-Ray Observations of the Young Pulsar J1357---6429 and Its Pulsar Wind Nebula \|Chang Chulhoon Pavlov George G. et al. \| ApJ \| 744-81 \| 2012 \| 2012ApJ...744...81C \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...744...81C Possible optical counterpart of PSR J1357-6429 \|Danilenko A. Kirichenko A. et al. \| A&A \| 540-28 \| 2012 \| 2012A&A...540A..28D \| http://ui.adsabs.harvard.edu/#abs/2012A&A...540A..28D Discovery of the source HESS J1356-645 associated with the young and energetic PSR J1357-6429 \|H.E.S.S. Collaboration Abramowski A. et al. \| A&A \| 533-103 \| 2011 \| 2011A&A...533A.103H \| http://ui.adsabs.harvard.edu/#abs/2011A&A...533A.103H Discovery of gamma- and X-ray pulsations from the young and energetic PSR J1357-6429 with Fermi and XMM-Newton \|Lemoine-Goumard M. Zavlin V. E. et al. \| A&A \| 533-102 \| 2011 \| 2011A&A...533A.102L \| http://ui.adsabs.harvard.edu/#abs/2011A&A...533A.102L 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 Suzaku observations of the old pulsar wind nebula candidate HESS J1356-645 \|Izawa Masaharu Dotani Tadayasu et al. \| PASJ \| 67-43 \| 2015 \| 2015PASJ...67...43I \| http://ui.adsabs.harvard.edu/#abs/2015PASJ...67...43I 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 Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz Tobias \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P 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 GeV Gamma-Ray Emission from Pulsar Wind Nebula HESS J1356-645 with Fermi-Large Area Telescope \|Liu Xi Guo Xiaolei et al. \| ApJ \| 942-105 \| 2023 \| 2023ApJ...942..105L \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...942..105L 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	2009-08-14T15:09:54Z/2009-08-15T14:44:08Z
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	2010-09-02T00:00:00Z
Last Update	2025-01-27
Keywords	"thermal emission", "fundamental physics", "elongated diffuse", "xmm newton", "ns surface", "chandra hrc", "compact pwn", "XMM-Newton", "neutron star interiors", "XMM", "psr j1357 6429", "deep imaging", "xray spectra", "thermal components", "provided tentative detections"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr George Pavlov, 2010, 'Young, hot PSR J1357-6429 and its PWN', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9b1wps0