A dataset provided by the European Space Agency

Name: Revisiting the Pulsar Injection Problem
Published: 2013-04-10T00:00:00Z

Proposal ID	067094
Title	Revisiting the Pulsar Injection Problem
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670940101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670940201
DOI	https://doi.org/10.5270/esa-anczg14
Principal Investigator, PI	Dr Slavko Bogdanov
Abstract	We propose XMM-Newton observations of three Galactic supernova remnants withpositionally coincident radio pulsars in order to confirm or refute theplausible connection between the supposedly old (but possibly very young)pulsars and the supernova remnants. Based on this we could (i) constrain theGalactic population of neutron stars born spinning slowly, (ii) determine anyconnection between the new class of so-called anti-magnetars and normal radiopulsars, (iii) extend the grossly incomplete X-ray catalog of Galactic supernovaremnants, and (iv) if the pulsars are not related to the remnants, look for acentral compact object and/or a pulsar wind nebula.
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 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 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	2012-03-20T08:40:08Z/2012-03-20T14:29:52Z
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	2013-04-10T00:00:00Z
Last Update	2025-01-27
Keywords	"normal radio pulsars", "pulsar wind nebula", "galactic supernova remnant", "xmm newton", "supernova remnant", "XMM-Newton", "galactic population", "pulsar injection", "XMM", "called anti magnetar", "central compact object"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Slavko Bogdanov, 2013, 'Revisiting the Pulsar Injection Problem', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-anczg14