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I review the basic observational properties of accreting millisecond pulsars that are important for understanding the physics involved in formation of their pulse profiles. I then discuss main effects responsible for shaping these profiles.…

Astrophysics · Physics 2008-11-27 Juri Poutanen

This study utilized the Tempotron, a robust classifier based on a third-generation neural network model, for pulse shape discrimination. By eliminating the need for manual feature extraction, the Tempotron model can process pulse signals…

Signal Processing · Electrical Eng. & Systems 2026-01-01 Haoran Liu , Peng Li , Ming-Zhe Liu , Kai-Ming Wang , Zhuo Zuo , Bing-Qi Liu

We present a new numerical algorithm for the calculation of pulse profiles from spinning neutron stars in the Hartle-Thorne approximation. Our approach allows us to formally take into account the effects of Doppler shifts and aberration, of…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Dimitrios Psaltis , Feryal Ozel

The detection of irregularly spaced pulses of non-negligible width is a fascinating yet under-explored topic in signal processing. It sits adjacent to other core topics such as radar and symbol detection yet has its own distinctive…

Signal Processing · Electrical Eng. & Systems 2025-03-11 Jonathan H. Manton

The n_TOF facility has just undergone in 2021 a major upgrade with the installation of its third generation spallation target that has been designed to optimize the performance of the two n_TOF time-of-flight lines. This contribution…

Nuclear Experiment · Physics 2023-06-21 J. Lerendegui-Marco , A. Casanovas , V. Alcayne , the n_TOF Collaboration

We report in this paper the proofs that the pulse shape analysis can be used in some bolometers to identify the nature of the interacting particle. Indeed, while detailed analyses of the signal time development in purely thermal detectors…

Nuclear Experiment · Physics 2015-05-20 C. Arnaboldi , C. Brofferio , O. Cremonesi , L. Gironi , M. Pavan , G. Pessina , S. Pirro , E. Previtali

Modeling the amplitudes and shapes of the X-ray pulsations observed from hot, rotating neutron stars provides a direct method for measuring neutron-star properties. This technique constitutes an important part of the science case for the…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Dimitrios Psaltis , Feryal Ozel , Deepto Chakrabarty

This article presents a few selected developments and future ideas related to the measurement of $(n,\gamma)$ data of astrophysical interest at CERN n_TOF. The MC-aided analysis methodology for the use of low-efficiency radiation detectors…

Nuclear Experiment · Physics 2023-02-07 C. Domingo-Pardo , V. Babiano-Suarez , J. Balibrea-Correa , L. Caballero , I. Ladarescu , J. Lerendegui-Marco , J. L. Tain , A. Tarifeño-Saldivia , O. Aberle , V. Alcayne , S. Altieri , S. Amaducci , J. Andrzejewski , M. Bacak , C. Beltrami , S. Bennett , A. P. Bernardes , E. Berthoumieux , M. Boromiza , D. Bosnar , M. Caamaño , F. Calviño , M. Calviani , D. Cano-Ott , A. Casanovas , F. Cerutti , G. Cescutti , S. Chasapoglou , E. Chiaveri , N. M. Chiera , P. Colombetti , N. Colonna , P. Console Camprini , G. Cortés , M. A. Cortés-Giraldo , L. Cosentino , S. Cristallo , S. Dellmann , M. Di Castro , S. Di Maria , M. Diakaki , M. Dietz , R. Dressler , E. Dupont , I. Durán , Z. Eleme , S. Fargier , B. Fernández , B. Fernández-Domínguez , P. Finocchiaro , S. Fiore , V. Furman , F. García-Infantes , A. Gawlik-Ramiega , G. Gervino , S. Gilardoni , E. González-Romero , C. Guerrero , F. Gunsing , C. Gustavino0 , J. Heyse , W. Hillman , D. G. Jenkins , E. Jericha , A. Junghans , Y. Kadi , K. Kaperoni , F. Käppeler , G. Kaur , A. Kimura , I. Knapová , U. Koester , M. Kokkoris , Y. Kopatch , M. Krtička , N. Kyritsis , C. Lederer-Woods , G. Lerner , A. Manna , T. Martínez , A. Masi , C. Massimi , P. Mastinu , M. Mastromarco , E. A. Maugeri , A. Mazzone , E. Mendoza , A. Mengoni , P. M. Milazzo , I. Mönch , R. Mucciola , F. Murtas , E. Musacchio-Gonzalez , A. Musumarra , A. Negret , A. Pérez de Rada , P. Pérez-Maroto , N. Patronis , J. A. Pavón-Rodríguez , M. G. Pellegriti , J. Perkowski , C. Petrone , E. Pirovano , J. Plaza , S. Pomp , I. Porras , J. Praena , J. M. Quesada , R. Reifarth , D. Rochman , Y. Romanets , C. Rubbia , A. Sánchez , M. Sabaté-Gilarte , P. Schillebeeckx , D. Schumann , A. Sekhar , A. G. Smith , N. V. Sosnin , M. Stamati , A. Sturniolo , G. Tagliente , D. Tarrío , P. Torres-Sánchez , J. Turko , S. Urlass , E. Vagena , S. Valenta , V. Variale , P. Vaz , G. Vecchio , D. Vescovi , V. Vlachoudis , R. Vlastou , T. Wallner , P. J. Woods , T. Wright , R. Zarrella , P. Žugec

A new Bayesian method for the analysis of folded pulsar timing data is presented that allows for the simultaneous evaluation of evolution in the pulse profile in either frequency or time, along with the timing model and additional…

Instrumentation and Methods for Astrophysics · Physics 2015-01-09 L Lentati , P. Alexander , M. P. Hobson

A new data analysis method is developed for the angle resolving silicon telescope introduced at the neutron time of flight facility n_TOF at CERN. The telescope has already been used in measurements of several neutron induced reactions with…

Data Analysis, Statistics and Probability · Physics 2020-06-14 P. Žugec , M. Barbagallo , J. Andrzejewski , J. Perkowski , N. Colonna , D. Bosnar , A. Gawlik , M. Sabate-Gilarte , M. Bacak , F. Mingrone , E. Chiaveri , M. Šako

We present an analytical study of light curves of slowly rotating radio pulsars with emphasis on the chromatic effects derived from the presence of a plasma environment; analyzing the effects of the compactness, the metric model, and the…

High Energy Astrophysical Phenomena · Physics 2023-02-27 Gastón Briozzo , Emanuel Gallo

A number of previous papers have developed an ion-proton theory of the pulsar polar cap. The basic equations summarizing this are given here with the results of sets of model step-to-step calculations of pulse-precursor profiles. The nature…

High Energy Astrophysical Phenomena · Physics 2020-01-08 P B Jones

In the framework of the ``ULTIMA'' project, we use ultra cold superfluid 3He bolometers for the direct detection of single particle events, aimed for a future use as a dark matter detector. One parameter of the pulse shape observed after…

Instrumentation and Detectors · Physics 2009-11-13 J. Elbs , Yu. M. Bunkov , E. Collin , H. Godfrin , O. Suvorova

We study a simple modification to the conventional time of flight mass spectrometry (TOFMS) where a \emph{variable} and (pseudo)-\emph{random} pulsing rate is used which allows for traces from different pulses to overlap. This modification…

Optimization and Control · Mathematics 2013-07-30 Morteza Ibrahimi , Andrea Montanari , George S Moore

Precision pulsar timing is integral to the detection of the nanohertz stochastic gravitational-wave background as well as understanding the physics of neutron stars. Conventional pulsar timing often uses fixed time and frequency-averaged…

Instrumentation and Methods for Astrophysics · Physics 2023-06-14 Rowina S. Nathan , Matthew T. Miles , Gregory Ashton , Paul D. Lasky , Eric Thrane , Daniel J. Reardon , Ryan M. Shannon , Andrew D. Cameron

It is believed that cores of neutron stars provide a natural laboratory where exotic high baryon density QCD phases may exist.The theoretically well established {\it neutron superfluid phase} is also believed to be found only inside neutron…

High Energy Astrophysical Phenomena · Physics 2024-06-25 Partha Bagchi , Oindrila Ganguly , Biswanath Layek , Anjishnu Sarkar , Ajit M. Srivastava

The Neutron Star Interior Composition Explorer (NICER) mission has provided a unique opportunity to constrain the equation of state of neutron stars by using the technique of pulse-profile modelling. This technique requires accurate and…

General Relativity and Quantum Cosmology · Physics 2021-05-12 G. André Oliva , Francisco Frutos-Alfaro

Ray tracing algorithms that compute pulse profiles from rotating neutron stars are essential tools for constraining neutron-star properties with data from missions such as NICER. However, the high computational cost of these simulations…

High Energy Astrophysical Phenomena · Physics 2025-06-16 Preston G. Waldrop , Dimitrios Psaltis , Tong Zhao

This paper presents a practical approach to digital pulse processing, emphasizing simplicity and efficiency. We advocate for a balanced software design, flat data structures, the use of the ROOT C++ interpreter, and a combination of…

Instrumentation and Detectors · Physics 2025-07-16 Jing Liu

This article presents a review about the main CERN n\_TOF contributions to the field of neutron-capture experiments of interest for $s$-process nucleosynthesis studies over the last 25 years, with special focus on the measurement of…

Nuclear Experiment · Physics 2025-02-17 C. Domingo-Pardo , O. Aberle , V. Alcayne , G. Alpar , M. Al Halabi , S. Amaducci , V. Babiano , M. Bacak , J. Balibrea-Correa , J. Bartolomé , A. P. Bernardes , B. Bernardino Gameiro , E. Berthoumieux , R. Beyer , M. Birch , M. Boromiza , D. Bosnar , B. Brusasco , M. Caamaño , A. Cahuzac , F. Calviño , M. Calviani , D. Cano-Ott , A. Casanovas , D. M. Castelluccio , D. Catlett , F. Cerutti , G. Cescutti , E. Chiaveri , G. Claps , P. Colombetti , N. Colonna , P. Console Camprini , G. Cortés , M. A. Cortés-Giraldo , L. Cosentino , S. Cristallo , A. D'Ottavi , G. de la Fuente Rosales , S. F. Dellmann , M. Diakaki , M. Di Castro , A. Di Chicco , M. Dietz , E. Dupont , I. Durán , Z. Eleme , M. Eslami , S. Fargier , B. Fernández-Domínguez , P. Finocchiaro , W. Flanagan , V. Furman , A. Gandhi , F. García-Infantes , A. Gawlik-Ramiega , G. Gervino , S. Gilardoni , E. González-Romero , S. Goula , E. Griesmayer , C. Guerrero , F. Gunsing , C. Gustavino , J. Heyse , W. Hillman , D. G. Jenkins , E. Jericha , A. Junghans , Y. Kadi , K. Kaperoni , I. Kelly , M. Kokkoris , Y. Kopatch , M. Krtička , N. Kyritsis , C. Lederer-Woods , J. Lerendegui-Marco , A. Manna , T. Martínez , M. Martínez-Cañada , A. Masi , C. Massimi , P. Mastinu , M. Mastromarco , E. A. Maugeri , A. Mazzone , E. Mendoza , A. Mengoni , V. Michalopoulou , P. M. Milazzo , J. Moldenhauer , R. Mucciola , E. Musacchio González , A. Musumarra , A. Negret , E. Odusina , D. Papanikolaou , N. Patronis , J. A. Pavón-Rodríguez , M. G. Pellegriti , P. Pérez-Maroto , A. Pérez de Rada Fiol , G. Perfetto , J. Perkowski , C. Petrone , N. Pieretti , L. Piersanti , E. Pirovano , I. Porras , J. Praena , J. M. Quesada , R. Reifarth , D. Rochman , Y. Romanets , A. Rooney , G. Rovira , C. Rubbia , A. Sánchez-Caballero , R. N. Sahoo , D. Scarpa , P. Schillebeeckx , A. G. Smith , N. V. Sosnin , M. Spelta , M. E. Stamati , K. Stasiak , G. Tagliente , A. Tarifeño-Saldivia , D. Tarrío , P. Torres-Sánchez , S. Tosi , G. Tsiledakis , S. Valenta , P. Vaz , G. Vecchio , D. Vescovi , V. Vlachoudis , R. Vlastou , A. Wallner , C. Weiss , P. J. Woods , T. Wright , R. Wu , P. Žugec , The n\_TOF Collaboration