Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-Ray Data Set-Reference-Cited by-同舟云学术

Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-Ray Data Set

Published:2019-12-12 Issue:1 Volume:887 Page:L25
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bogdanov Slavko^ORCID,Guillot Sebastien^ORCID,Ray Paul S.^ORCID,Wolff Michael T.^ORCID,Chakrabarty Deepto^ORCID,Ho Wynn C. G.^ORCID,Kerr Matthew^ORCID,Lamb Frederick K.^ORCID,Lommen Andrea,Ludlam Renee M.^ORCID,Milburn Reilly,Montano Sergio,Miller M. Coleman^ORCID,Bauböck Michi,Özel Feryal,Psaltis Dimitrios^ORCID,Remillard Ronald A.,Riley Thomas E.^ORCID,Steiner James F.^ORCID,Strohmayer Tod E.^ORCID,Watts Anna L.^ORCID,Wood Kent S.,Zeldes Jesse,Enoto Teruaki^ORCID,Okajima Takashi,Kellogg James W.,Baker Charles,Markwardt Craig B.^ORCID,Arzoumanian Zaven,Gendreau Keith C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/ab53eb/pdf

Reference110 articles.

1. GW170817: Measurements of Neutron Star Radii and Equation of State

2. A new class of radio pulsars

3. The NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars

4. Discovery of Four Isolated Millisecond Pulsars

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