An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451
Astronomical Institute of the Slovak Academy of Sciences · University of Amsterdam · +12 more institutions
Abstract
Abstract In 2019 the NICER collaboration published the first mass and radius inferred for PSR J0030+0451, thanks to NICER observations, and consequent constraints on the equation of state characterizing dense matter. Two independent analyses found a mass of ∼1.3–1.4 M ⊙ and a radius of ∼13 km. They also both found that the hot spots were all located on the same hemisphere, opposite to the observer, and that at least one of them had a significantly elongated shape. Here we reanalyze, in greater detail, the same NICER data set, incorporating the effects of an updated NICER response matrix and using an upgraded analysis framework. We expand the adopted models and also jointly analyze XMM-Newton data, which…
Citation impact
- FWCI
- 56.67
- Percentile
- 100%
- References
- 60
Authors
15- SVS. VinciguerraCorresponding
Astronomical Institute of the Slovak Academy of Sciences, University of Amsterdam
- TSTuomo Salmi
Astronomical Institute of the Slovak Academy of Sciences, University of Amsterdam
- ALAnna L. Watts
Astronomical Institute of the Slovak Academy of Sciences, University of Amsterdam
- DCDevarshi Choudhury
Astronomical Institute of the Slovak Academy of Sciences, University of Amsterdam
- TEThomas E. Riley
Astronomical Institute of the Slovak Academy of Sciences, University of Amsterdam
Topics & keywords
- Physics
- RADIUS
- Astrophysics
Funding
- NANational Aeronautics and Space AdministrationAward: 80NSSC22K0728
- ECEuropean CommissionAward: 865768 AEONS
- CNCentre National d’Etudes Spatiales
- NONederlandse Organisatie voor Wetenschappelijk Onderzoek
- NSNuclear Safety and Security Commission
- NSNatural Sciences and Engineering Research Council of CanadaAwards: 2019-06077, 06077, RGPIN-2019, RGPIN-2019-06077