M
M. C. Miller
Researcher at University of Maryland, College Park
Publications - 49
Citations - 4024
M. C. Miller is an academic researcher from University of Maryland, College Park. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 24, co-authored 49 publications receiving 2922 citations.
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Journal ArticleDOI
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
M. C. Miller,Frederick K. Lamb,Alexander J. Dittmann,Slavko Bogdanov,Zaven Arzoumanian,Keith C. Gendreau,Sebastien Guillot,Alice K. Harding,Wynn C. G. Ho,Wynn C. G. Ho,James M. Lattimer,Renee M. Ludlam,Simin Mahmoodifar,Simin Mahmoodifar,Sharon M. Morsink,Paul S. Ray,Tod E. Strohmayer,K. S. Wood,Teruaki Enoto,R. S. Foster,Takashi Okajima,Gregory Y. Prigozhin,Yang Soong +22 more
TL;DR: In this paper, the mass and radius of the isolated 205.53 Hz millisecond pulsar PSR J0030+0451 were estimated using a Bayesian inference approach to analyze its energy-dependent thermal X-ray waveform, which was observed using the Neutron Star Interior Composition Explorer (NICER).
Journal ArticleDOI
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
M. C. Miller,Frederick K. Lamb,Alexander J. Dittmann,Slavko Bogdanov,Zaven Arzoumanian,Keith C. Gendreau,Sebastien Guillot,Alice K. Harding,Wynn C. G. Ho,Wynn C. G. Ho,James M. Lattimer,Renee M. Ludlam,Simin Mahmoodifar,Simin Mahmoodifar,Sharon M. Morsink,Paul S. Ray,Tod E. Strohmayer,K. S. Wood,Teruaki Enoto,R. S. Foster,Takashi Okajima,Gregory Y. Prigozhin,Yang Soong +22 more
TL;DR: In this article, the mass and radius of the isolated 205.53 Hz millisecond pulsar PSR J0030+0451 were estimated using a Bayesian inference approach to analyze its energy-dependent thermal X-ray waveform.
Journal ArticleDOI
The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
M. C. Miller,Frederick K. Lamb,Alexander J. Dittmann,Slavko Bogdanov,Zaven Arzoumanian,Keith C. Gendreau,Sebastien Guillot,Sebastien Guillot,Wynn C. G. Ho,James M. Lattimer,Michael Loewenstein,Michael Loewenstein,Sharon M. Morsink,Paul S. Ray,Michael T. Wolff,Charles Baker,Thoniel Cazeau,Sridhar S. Manthripragada,C. B. Markwardt,Takashi Okajima,S. Pollard,Ismaël Cognard,Ismaël Cognard,H. T. Cromartie,Emmanuel Fonseca,Lucas Guillemot,Lucas Guillemot,Matthew Kerr,Aditya Parthasarathy,Timothy T. Pennucci,Timothy T. Pennucci,Scott M. Ransom,Ingrid H. Stairs +32 more
TL;DR: In this article, the authors reported a radius measurement based on fits of rotating hot spot patterns to Neutron Star Interior Composition Explorer (NICER) and X-ray Multi-Mirror (XMM-Newton) observations.
Journal ArticleDOI
X-Ray Spectroscopic Evidence for Intermediate-Mass Black Holes: Cool Accretion Disks in Two Ultraluminous X-Ray Sources
TL;DR: In this paper, an XMM-Newton observation of the nearby spiral galaxy NGC 1313, which contains two ultraluminous X-ray (ULX) sources, was analyzed, and the soft components in these ULX spectra were well fitted by multicolor disk blackbody models with color temperatures of kT 150 eV.
Journal ArticleDOI
X-ray Spectroscopic Evidence for Intermediate Mass Black Holes: Cool Accretion Disks in Two Ultra--Luminous X-ray Sources
TL;DR: In this article, the authors analyzed an XMM-Newton observation of the nearby spiral galaxy NGC 1313, which contains two "ultra-luminous" X-ray (ULX) sources.