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The NASA Neutron star Interior Composition Explorer (\emph{NICER}) mission measures the X-ray pulse profiles of select millisecond pulsars and uses sophisticated pulse profile modeling (PPM) techniques to constrain their masses ($M$) and…

High Energy Astrophysical Phenomena · Physics 2026-04-14 Ryan O'Connor , Chun Huang , Alexander Y. Chen

NASA's Neutron Star Interior Composition Explorer (NICER) observed X-ray emission from the pulsar PSR J0030+0451 in 2018. Riley et al. reported Bayesian parameter measurements of the mass and the star's radius using pulse-profile modeling…

High Energy Astrophysical Phenomena · Physics 2024-02-02 Chaitanya Afle , Patrick R. Miles , Silvina Caino-Lores , Collin D. Capano , Ingo Tews , Karan Vahi , Ewa Deelman , Michela Taufer , Duncan A. Brown

Modeling energy-dependent X-ray pulse profiles from rotation-powered millisecond pulsars observed with NICER has emerged as a promising avenue for measuring neutron star radii and probing the equation of state of cold, ultra-dense matter.…

High Energy Astrophysical Phenomena · Physics 2026-01-06 Tolga Guver , Dimitrios Psaltis , Feryal Ozel , Tong Zhao

We report the detection of 376.05 Hz (2.66 ms) coherent X-ray pulsations in NICER observations of a transient outburst of the low-mass X-ray binary IGR J17494-3030 in 2020 October/November. The system is an accreting millisecond X-ray…

Both the mass and radius of the millisecond pulsar PSR J0030+0451 have been inferred via pulse-profile modeling of X-ray data obtained by NASA's NICER mission. In this Letter we study the implications of the mass-radius inference reported…

The observation of neutron stars enables the otherwise impossible study of fundamental physical processes. The timing of binary radio pulsars is particularly powerful, as it enables precise characterization of their (three-dimensional)…

NICER observed several rotation-powered millisecond pulsars to search for or confirm the presence of X-ray pulsations. When broad and sine-like, these pulsations may indicate thermal emission from hot polar caps at the magnetic poles on the…

In the last few years, the NICER collaboration has provided mass and radius inferences, via pulse profile modeling, for two pulsars: PSR J0030+0451 and PSR J0740+6620. Given the importance of these results for constraining the equation of…

High Energy Astrophysical Phenomena · Physics 2024-01-09 Serena Vinciguerra , Tuomo Salmi , Anna L. Watts , Devarshi Choudhury , Yves Kini , Thomas E. Riley

Four neutron star radius measurements have already been obtained by modeling the X-ray pulses of rotation-powered millisecond pulsars observed by the Neutron Star Interior Composition ExploreR (NICER). We report here the radius measurement…

We report on the timing and spectral properties of PSR J1838-0655 using joint observations from the Neutron Star Interior Composition Explorer (NICER) and the Nuclear Spectroscopic Telescope Array (NuSTAR). By disentangling the pulsar's…

High Energy Astrophysical Phenomena · Physics 2025-08-27 Xian-Ao Wang , Han-Long Peng , Jin-Tao Zheng , Shi-Qi Zhou , Wen-Tao Ye , Ming-Yu Ge , Xiang-Hua Li , Shi-Jie Zheng

Thermal X-ray emission from rotation-powered millisecond pulsars, shaped by gravitational lensing and the beaming of the surface radiation, provides critical insights into neutron star properties. This approach has been the focus of…

High Energy Astrophysical Phenomena · Physics 2025-07-31 Tong Zhao , Dimitrios Psaltis , Feryal Ozel

We have used X-ray data from the Neutron Star Interior Composition Explorer (NICER) to search for long time-scale, correlated variations ("red noise") in the pulse times of arrival from the millisecond pulsars PSR J1824$-$2452A and PSR…

We report on the Neutron Star Interior Composition Explorer (NICER) monitoring campaign of the 468 Hz accreting millisecond X-ray pulsar IGR J17379-3747. From a detailed spectral and timing analysis of the coherent pulsations we find that…

We study the effects of the time-variable properties of thermonuclear X-ray bursts on modeling their millisecond-period burst oscillations. We apply the pulse profile modeling technique that is being used in the analysis of rotation-powered…

High Energy Astrophysical Phenomena · Physics 2023-04-12 Yves Kini , Tuomo Salmi , Anna L. Watts , Serena Vinciguerra , Devarshi Choudhury , Siem Fenne , Slavko Bogdanov , Zach Meisel , Valery Suleimanov

The X-ray pulsar RX J0440.9+4431 went through a giant outburst in 2022 and reached a record-high flux of 2.3 Crab, as observed by Swift/BAT. We study the evolution of different spectral and timing properties of the source using NICER…

Recent constraints on neutron star mass and radius have advanced our understanding of the equation of state (EOS) of cold dense matter. Some of them have been obtained by modeling the pulses of three millisecond X-ray pulsars observed by…

We report Bayesian inference of the mass, radius and hot X-ray emitting region properties - using data from the Neutron Star Interior Composition ExploreR (NICER) - for the brightest rotation-powered millisecond X-ray pulsar PSR…

Understanding the existence of exotic matter phases and phase transitions within the core of neutron stars is crucial to advancing our knowledge of cold-dense matter physics. Recent multi-messenger observations, including gravitational…

High Energy Astrophysical Phenomena · Physics 2025-05-07 Chun Huang , Shashwat Sourav

Current space missions primarily depend on Earth-based Guidance, Navigation, and Control (GNC) systems involving human-in-the-loop operations. X-ray pulsar-based navigation offers a promising alternative by using the very precise periodic…

Instrumentation and Methods for Astrophysics · Physics 2026-04-22 Sui Chen , Emilie Parent , Nanda Rea , Francesco Topputo

We have simulated the X-ray polarization data that can be obtained with the Imaging X-ray Polarimetry Explorer, when observing accretion-powered millisecond pulsars. We estimated the necessary exposure times for SAX J1808.4$-$3658 in order…

High Energy Astrophysical Phenomena · Physics 2021-02-03 Tuomo Salmi , Vladislav Loktev , Karri Korsman , Luca Baldini , Sergey S. Tsygankov , Juri Poutanen