A dataset provided by the European Space Agency

Name: Deep XMM-Newton Observation of the Relativistic Double Pulsar PSR J0737-3039
Published: 2007-11-28T00:00:00Z

Proposal ID	040510
Title	Deep XMM-Newton Observation of the Relativistic Double Pulsar PSR J0737-3039
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405100101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405100201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405100301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405100401
DOI	https://doi.org/10.5270/esa-oxauyh1
Principal Investigator, PI	Dr Alberto Pellizzoni
Abstract	The binary radio pulsar J0737-3039 is a truly unique system offering theenormous diagnostics of two radio pulsars in a short orbital period system. Theproperties of these two neutron stars are being constrained with unprecedentedprecision. In particular, this system is a unique laboratory for the study ofthe pulsar magnetospheres and the interaction between the pulsars relativisticwinds. High-energy observations are necessary to give a complete picture of theprocesses. The low X-ray luminosity requires a very long exposure time, but theadded value of the detailed modeling of these pulsars through observation atother wavelengths, makes this a worth investment. No other X-ray observatory ofthe current generation will be able to yield better information.
Publications	PSR J0737-3039: Interacting Pulsars in X-Rays \|Pellizzoni A. Tiengo A. et al. \| ApJ \| 679-664 \| 2008 \| 2008ApJ...679..664P \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...679..664P An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi J. A. Albacete Colombo J. F. et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C Long-term X-ray timing of the double pulsar PSR J0737-3039 \|Iacolina M. N. Pellizzoni A. \| AN \| 335-324 \| 2014 \| 2014AN....335..324I \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..324I Automatic Classification of Time-variable X-Ray Sources \|Lo Kitty K. Farrell Sean et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Long-term Study of the Double Pulsar J0737-3039 with XMM-Newton: Spectral Analysis \|Egron E. Pellizzoni A. et al. \| ApJ \| 838-120 \| 2017 \| 2017ApJ...838..120E \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...838..120E An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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 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	2006-10-26T00:45:45Z/2006-10-29T11:20:32Z
Version	PPS_NOT_AVAILABLE
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	2007-11-28T00:00:00Z
Last Update	2025-01-27
Keywords	"exposure time", "added value", "radio pulsars", "neutron stars", "pulsar magnetosphere", "XMM-Newton", "complete picture", "worth investment", "relativistic winds", "XMM", "xray observatory", "deep xmm newton", "low xray luminosity"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alberto Pellizzoni, 2007, 'Deep XMM-Newton Observation of the Relativistic Double Pulsar PSR J0737-3039', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-oxauyh1