activity
20082026
most citedThe Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

4.1k citations · 35.4k across the 240 of their papers we have counts for

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Showing astro-ph.HEShow all

200 papers · 1 filter

astro-ph.HE2026

Science Using Single-Pulse Exploration with Combined Telescopes: II. Pulse profile evolution and single-pulse modulation

F. Jankowski, J. -M. Griessmeier, T. Roy +11

Aims. We aim to illuminate how the pulsars' integrated pulse profiles and single-pulse modulation evolve with radio frequency, while separating intrinsic and propagation effects. M…

astro-ph.HE2026

Searching for optical pulsations from spider millisecond pulsars with the fast photometer SiFAP2

Christian Malacaria, Alessandro Papitto, Filippo Ambrosino +19

Optical pulsations from millisecond pulsars (MSPs) have recently been detected in a transitional MSP and an accreting MSP. Evidence for optical pulsations has also been found for a…

astro-ph.HE2026

A NICER view of PSR J16142230: a massive and compact millisecond pulsar

Lucien Mauviard, Sebastien Guillot, Lami Suleiman +17

Using pulse profile modeling, we obtain the mass-radius measurement of a millisecond pulsar (MSP) with data from the Neutron Star Interior Composition ExploreR, XMM-Newton and the…

astro-ph.HE2026

Generalized Non-linear Bayesian Pulsar Timing with Enterprise

Andrew R. Kaiser, Jeffrey S. Hazboun, Maura A. McLaughlin +56

In this study, we use the Bayesian methods in the Enterprise package to examine the fully general parameterization of pulsar timing models in tandem with noise. We investigate four…

astro-ph.HE2026

A NICER view of the millisecond pulsar PSR J21243358: evidence for a helium atmosphere

Denis González-Caniulef, Sebastien Guillot, Pierre Stammler +12

Pulse profile modeling has proven to be a powerful technique for determining the mass and radius of neutron stars. To date, this method has been applied to a handful of millisecond…

astro-ph.HE2026★ 1 cited

On the polarization position angle jumps in FRB 20240114A

Ninisha Manaswini, Danté M. Hewitt, Laura G. Spitler +6

Fast radio bursts (FRBs), thought to originate from magnetars, exhibit diverse polarization properties that constrain their emission physics and local magneto-ionic environments. T…

astro-ph.HE2026★ 2 cited

Multi-wavelength emission modelling of PSR~J04374715

J. Pétri, P. Stammler, L. Guillemot +4

The diversity of pulsar light-curves and radio polarisation properties originates in the structure of the magnetic field close to the stellar surface. For millisecond pulsars, this…

astro-ph.HE2025

A glitch in the millisecond pulsar J09003144

Bhavnesh Bhat, Michael J. Keith, Ismaël Cognard +11

We report the detection of a glitch in the millisecond pulsar (MSP) PSR J09003144, which is included in the European, MeerKAT and Parkes pulsar timing array experiments. The dat…

astro-ph.HE2025★ 1 cited

Shapiro Delay Measurements from Fifteen Years of PSR J12311411 Radio Observations

H. Thankful Cromartie, Matthew Kerr, Scott M. Ransom +5

We present 15 years of Nançay and Green Bank radio telescope timing observations for PSR J12311411. This millisecond pulsar is a primary science target for the Neutron Star Inte…

astro-ph.HE2025

Revisiting FRB 20121102A: milliarcsecond localisation and a decreasing dispersion measure

M. P. Snelders, J. W. T. Hessels, J. Huang +27

FRB 20121102A is the original repeating fast radio burst (FRB) source and also the first to be localised to milliarcsecond precision using very-long-baseline interferometry (VLBI).…

astro-ph.HE2025★ 6 cited

A double dipole geometry for PSR~J0740+6620

J. Pétri, S. Guillot, L. Guillemot +5

Millisecond pulsars are known to show complex radio pulse profiles and polarisation position angle evolution with rotational phase. Small scale surface magnetic fields and multipol…

astro-ph.HE2025★ 53 cited

A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329

Lucien Mauviard, Sebastien Guillot, Tuomo Salmi +20

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 Composit…

astro-ph.HE2025★ 1 cited

The polarimetric response of the Nançay Radio Telescope and its impact on precision pulsar timing

Lucas Guillemot, Willem van Straten, Ismaël Cognard +3

In \citet{Guillemot2023} we presented a new method for calibrating pulsar observations conducted with the Nançay decimetric Radio Telescope (NRT), which significantly improved NRT…

astro-ph.HE2025★ 3 cited

A census of galactic spider binary millisecond pulsars with the Nançay Radio Telescope

Clara Blanchard, Lucas Guillemot, Guillaume Voisin +2

Spider pulsars are systems in which a millisecond pulsar (MSP) tightly orbits (Pb 1 day) a low mass (mc 0.5 M) semi-degenerate star. Spider often disp…

astro-ph.HE2024

The impact on astrometry by solar-wind effect in pulsar timing

K. Liu, A. Parthasarathy, M. Keith +16

Astrometry of pulsars, particularly their distances, serves as a critical input for various astrophysical experiments using pulsars. Pulsar timing is a primary approach for determi…

astro-ph.HE2024

Search for Extended GeV Sources in the Inner Galactic Plane

S. Abdollahi, F. Acero, A. Acharyya +108

The recent detection of extended -ray emission around middle-aged pulsars is interpreted as inverse-Compton scattering of ambient photons by electron-positron pairs escaping the…

astro-ph.HE2024★ 1 cited

Explanation of the exceptionally strong timing noise of PSR J0337+1715 by a circum-ternary planet and consequences for gravity tests

Guillaume Voisin, Ismaël Cognard, Melaine Saillenfest +6

Context: Timing of pulsar PSR J0337+1715 provides a unique opportunity to test the strong equivalence principle (SEP) with a strongly self-gravitating object. This is due to its un…

astro-ph.HE2024★ 5 cited

Impact of the observation frequency coverage on the significance of a gravitational wave background detection in PTA data

Irene Ferranti, Mikel Falxa, Alberto Sesana +8

Pulsar Timing Array (PTA) collaborations gather high-precision timing measurements of pulsars with the aim of detecting gravitational wave (GW) signals. A major challenge lies in t…

astro-ph.HE2024

A Repeating Fast Radio Burst Source in a Low-Luminosity Dwarf Galaxy

Danté M. Hewitt, Mohit Bhardwaj, Alexa C. Gordon +48

We present the localization and host galaxy of FRB 20190208A, a repeating source of fast radio bursts (FRBs) discovered using CHIME/FRB. As part of the PRECISE repeater localizatio…

astro-ph.HE2024★ 1 cited

Triple trouble with PSR J1618-3921: Mass measurements and orbital dynamics of an eccentric millisecond pulsar

K. Grunthal, V. Venkatraman Krishnan, P. C. C. Freire +11

PSR J1618-3921 is one of five known millisecond pulsars (MSPs) in eccentric orbits (eMPSs) located in the Galactic plane, whose formation is poorly understood. Earlier studies of t…

astro-ph.HE2024★ 86 cited

A NICER View of PSR J12311411: A Complex Case

Tuomo Salmi, Julia S. Deneva, Paul S. Ray +16

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…

astro-ph.HE2024

Periodicity search in the timing of the 25 millisecond pulsars from the second data release of the European Pulsar Timing Array

Iuliana Nitu, Michael Keith, David Champion +17

In this work, we investigated the presence of strictly periodic, as well as quasi-periodic signals, in the timing of the 25 millisecond pulsars from the EPTA DR2 dataset. This is e…

astro-ph.HE2024★ 2 cited

Localisation of the non-thermal X-ray emission of PSR~J2229+6114 from its multi-wavelength pulse profiles

J. Pétri, S. Guillot, L. Guillemot +5

Pulsars are detected over the whole electromagnetic spectrum, from radio wavelengths up to very high energies, in the GeV-TeV range. Whereas the radio emission site for young pulsa…

astro-ph.HE2024

The NANOGrav 15 yr Data Set: Chromatic Gaussian Process Noise Models for Six Pulsars

Bjorn Larsen, Chiara M. F. Mingarelli, Jeffrey S. Hazboun +61

Pulsar timing arrays (PTAs) are designed to detect low-frequency gravitational waves (GWs). GWs induce achromatic signals in PTA data, meaning that the timing delays do not depend…