A dataset provided by the European Space Agency

Name: A simultaneous X-ray and radio observation of the nearby pulsar B1133+16.
Published: 2015-07-23T22:00:00Z

Proposal ID	074114
Title	A simultaneous X-ray and radio observation of the nearby pulsar B1133+16.
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741140201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741140301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741140401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741140501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0741140601
DOI	https://doi.org/10.5270/esa-xspsu6f
Principal Investigator, PI	Prof Janusz Gil
Abstract	The activity of the inner acceleration gap in pulsars should be detectable inboth thermal and non-thermal X-rays. The electron-positron pair plasma ispolarised by the accelerating electric field. One species bombards the surfaceand heats the polar cap to MK temperatures, while the other one creates thesecondary plasma in the magnetosphere. The old cool pulsars should be detectedin X-rays as thermal blackbody (BB) radiation from hot polar cap, together withnon-thermal synchrotron radiation originating far from the surface. We propose asensitive 100 ks exposure observation by XMM-Newton simultaneous withGMRT/Effelsberg radio observations of the nearby pulsar B1133+16, to preciselydetermine the X-ray signatures of its inner acceleration region.
Publications	XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N 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 XMM-Newton Observation of the nearby Pulsar B1133+16. \|Szary, Andrzej, Gil, Janusz, et al. \| ApJ \| 835-178 \| 2017 \| 2017ApJ...835..178S \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...835..178S A new X-ray look into four old pulsars \|Rigoselli, Michela, Mereghetti, Sandro, \| A&A \| 615-73 \| 2018 \| 2018A&A...615A..73R \| http://ui.adsabs.harvard.edu/#abs/2018A&A...615A..73R 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 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	2014-05-25T12:18:42Z/2014-06-28T17:55:32Z
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	2015-07-23T22:00:00Z
Keywords	"polar cap", "species bombards", "secondary plasma", "inner acceleration gap", "nearby pulsar b1133", "XMM", "cool pulsars", "nonthermal xray", "hot polar cap", "xray signatures", "XMM-Newton", "effelsberg radio", "accelerating electric field", "inner acceleration region", "nonthermal synchrotron radiation", "mk temperatures", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Janusz Gil, 2015, 'A simultaneous X-ray and radio observation of the nearby pulsar B1133+16.', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xspsu6f