A dataset provided by the European Space Agency

Name: Long Term X-ray Monitoring of the Double Pulsar PSR J0737-3039
Published: 2013-01-24T00:00:00Z

Proposal ID	067081
Title	Long Term X-ray Monitoring of the Double Pulsar PSR J0737-3039
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670810101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670810201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670810301
DOI	https://doi.org/10.5270/esa-b9jpmfe
Principal Investigator, PI	Dr Alberto Pellizzoni
Abstract	Clear evidences of orbital phase-dependent interactions between the two pulsarsof the relativistic double neutron star binary PSR J0737-3039 are seen both inradio and X-rays observations. In particular, XMM recently discovered the X-raybrightening of PSR B via energy transfer from PSR A, a process probablycorrelated with the strong radio intensity fluctuations of PSR B seen along theorbit. No other X-ray observatory of the current generation (or foreseen withinthe next decade) will be able to yield better information, and considering thedisappearance of PSR B (March 2008) in the radio band, XMM offers the exclusiveopportuinity to monitor this evolving pulsar and its related neutron starsurface thermodynamics.
Publications	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 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 Long-term Study of the Double Pulsar J0737--3039 with XMM-Newton: Pulsar Timing \|Iacolina, M. N., Pellizzoni, A., et al. \| ApJ \| 824-87 \| 2016 \| 2016ApJ...824...87I \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...824...87I 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 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 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	2011-10-22T20:36:18Z/2011-10-28T08:16:04Z
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	2013-01-24T00:00:00Z
Keywords	"evolving pulsar", "exclusive opportuinity", "via energy transfer", "XMM", "xray brightening", "radio intensity fluctuations", "xray observatory", "term xray", "radio band"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alberto Pellizzoni, 2013, 'Long Term X-ray Monitoring of the Double Pulsar PSR J0737-3039', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-b9jpmfe