A dataset provided by the European Space Agency

Name: Constraining the Equation of State of the Neutron Star PSR J0437-4715
Published: 2011-01-13T00:00:00Z

Proposal ID	060346
Title	Constraining the Equation of State of the Neutron Star PSR J0437-4715
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0603460101
DOI	https://doi.org/10.5270/esa-od86m0i
Principal Investigator, PI	Dr Slavko Bogdanov
Abstract	Modeling of thermal X-ray spectra and pulse profiles of radio millisecondpulsars (MSPs) may offer important insight into neutron star structure. As thenearest and brightest MSP, PSR J0437--4715 can be studied in most detail andthus provide the best constraints. Unfortunately, due to the unfavorableobserving roll angle, the existing XMM-Newton timing data from this pulsar aresignificantly contaminated by a nearby bright AGN. We propose a better optimizedand deeper XMM-Newton study of PSR J0437--4715, which could result in a majoradvance towards constraining the neutron star equation of state.
Publications	The Nearest Millisecond Pulsar Revisited with XMM-Newton: Improved Mass-radius Constraints for PSR J0437-4715 \|Bogdanov Slavko \| ApJ \| 762-96 \| 2013 \| 2013ApJ...762...96B \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...762...96B 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 Is HE 0436-4717 Anemic? A deep look at a bare Seyfert 1 galaxy \|Bonson K. Gallo L. C. \| MNRAS \| 450-857 \| 2015 \| 2015MNRAS.450..857B \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.450..857B The NuSTAR view of the non-thermal emission from PSR J0437-4715 \|Guillot S. Kaspi V. M. et al. \| MNRAS \| 463-2612 \| 2016 \| 2016MNRAS.463.2612G \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.2612G 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 Constraining the Neutron Star Massu2500Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-Ray Data Set \|Bogdanov Slavko Guillot Sebastien et al. \| ApJ \| 887-25 \| 2019 \| 2019ApJ...887L..25B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887L..25B 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 Tidal deformability of quark stars with repulsive interactions \|Albino M. B. Fariello R. \| PhRvD \| 104-83011 \| 2021 \| 2021PhRvD.104h3011A \| http://ui.adsabs.harvard.edu/#abs/2021PhRvD.104h3011A Relativistic force-free models of the thermal X-ray emission in millisecond pulsars observed by NICER \|Carrasco F. Pelle J. et al. \| MNRAS \| 520-3151 \| 2023 \| 2023MNRAS.520.3151C \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.520.3151C 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	2009-12-15T19:40:32Z/2009-12-17T07:36:57Z
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	2011-01-13T00:00:00Z
Last Update	2025-01-27
Keywords	"existing xmm newton", "roll angle", "nearby bright agn", "XMM-Newton", "pulse profiles", "thermal xray spectra", "neutron star structure", "psr j0437 4715", "deeper xmm newton", "neutron star equation", "brightest msp", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Slavko Bogdanov, 2011, 'Constraining the Equation of State of the Neutron Star PSR J0437-4715', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-od86m0i