A dataset provided by the European Space Agency

Name: Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451
Published: 2009-01-24T00:00:00Z

Proposal ID	050229
Title	Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502290101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502290201
DOI	https://doi.org/10.5270/esa-ei1bukj
Principal Investigator, PI	Mr Slavko Bogdanov
Abstract	Modeling the thermal X-ray spectra and pulse profiles of radio millisecondpulsars (MSPs) provides important insight into the properties of neutron stars(NSs). In the nearest MSP, J0437--4715, with such modeling we are able to placeconstraints on the mass-to-radius ratio of the star, the B-field geometry, andsurface properties. Application of this powerful method on another system wouldprovide a crucial validity check and allow an additional set of measuremens. AnXMM-Newton X-ray study of the nearby PSR J0030+0451, may lead to a major advancetowards constraining the NS equation of state and other important NS parameters.
Publications	Deep XMM-Newton Spectroscopic and Timing Observations of the Isolated Radio Millisecond Pulsar PSR J0030+0451 \|Bogdanov Slavko Grindlay Jonathan E. \| ApJ \| 703-1557 \| 2009 \| 2009ApJ...703.1557B \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...703.1557B A Multiwavelength Study on the High-energy Behavior of the Fermi/LAT Pulsars \|Marelli Martino De Luca Andrea \| ApJ \| 733-82 \| 2011 \| 2011ApJ...733...82M \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...733...82M 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 Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc N. Sadibekova T. et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C 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 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 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 Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti F. Middei R. et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V 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 SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc N. Merloni A. et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation \|Riley T. E. Watts A. L. et al. \| ApJ \| 887-21 \| 2019 \| 2019ApJ...887L..21R \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887L..21R PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter \|Miller M. C. Lamb F. K. et al. \| ApJ \| 887-24 \| 2019 \| 2019ApJ...887L..24M \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887L..24M 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 X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham Mona Clerc Nicolas et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba Matej Lieu Maggie et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc N. Kirkpatrick C. C. et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C 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 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 A Nuclear Equation of State Inferred from Stellar r-process Abundances \|Holmbeck Erika M. OShaughnessy Richard et al. \| ApJ \| 926-196 \| 2022 \| 2022ApJ...926..196H \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...926..196H 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 Unified nuclear matter equations of state constrained by the in-medium balance in density-dependent covariant density functionals \|Xia Cheng-Jun Sun Bao Yuan et al. \| PhRvC \| 105-45803 \| 2022 \| 2022PhRvC.105d5803X \| http://ui.adsabs.harvard.edu/#abs/2022PhRvC.105d5803X The Effect of f(R T) Modified Gravity on the Mass and Radius of Pulsar HerX1 \|Nashed G. G. L. \| ApJ \| 950-129 \| 2023 \| 2023ApJ...950..129N \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...950..129N Atmospheric Effects on Neutron Star Parameter Constraints with NICER \|Salmi Tuomo Vinciguerra Serena et al. \| ApJ \| 956-138 \| 2023 \| 2023ApJ...956..138S \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...956..138S An Updated Mass-Radius Analysis of the 2017-2018 NICER Data Set of PSR J0030+0451 \|Vinciguerra Serena Salmi Tuomo et al. \| ApJ \| 961-62 \| 2024 \| 2024ApJ...961...62V \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961...62V Crossover equation of state based on color-molecular-dynamics \|Yasutake Nobutoshi Maruyama Toshiki \| PhRvD \| 109-043056 \| 2024 \| 2024PhRvD.109d3056Y \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109d3056Y Gravitational-wave imprints of nonconvex dynamics in binary neutron star mergers \|Rivieccio Giuseppe Guerra Davide et al. \| PhRvD \| 109-064032 \| 2024 \| 2024PhRvD.109f4032R \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109f4032R Bulk Properties of PSR J0030+0451 Inferred with the Compactness Measurement of NICER \|Luo Chuan-Ning Tang Shao-Peng et al. \| ApJ \| 966-98 \| 2024 \| 2024ApJ...966...98L \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966...98L 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 Extended Skyrme effective interactions for transport models and neutron stars \|Wang Si-Pei Wang Rui et al. \| PhRvC \| 109-054623 \| 2024 \| 2024PhRvC.109e4623W \| http://ui.adsabs.harvard.edu/#abs/2024PhRvC.109e4623W Thermal x-ray studies of neutron stars and the equation of state \|Miao Zhiqiang Qi Liqiang et al. \| PhRvD \| 109-123005 \| 2024 \| 2024PhRvD.109l3005M \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109l3005M
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2007-12-12T20:15:05Z/2007-12-14T08:50:34Z
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	2009-01-24T00:00:00Z
Last Update	2025-01-27
Keywords	"ns equation", "millisecond pulsar j0030", "powerful method", "j0437 4715", "neutron stars nss", "surface properties", "XMM-Newton", "radius ratio measurement", "xmm newton xray", "thermal xray spectra", "radius ratio", "pulse profiles", "ns parameters", "nearby psr j0030", "validity check", "XMM", "field geometry", "additional set"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Slavko Bogdanov, 2009, 'Mass-to-Radius Ratio Measurement of the Millisecond Pulsar J0030+0451', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ei1bukj