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We have compiled a new and complete catalog of the main properties of the 1509 pulsars for which published information currently exists. The catalog includes all spin-powered pulsars as well as anomalous X-ray pulsars and soft gamma-ray repeaters showing coherent pulsed emission, but excludes accretion-powered systems. References are given for all data listed. We have also developed a new web interface for accessing and displaying either tabular or plotted data with the option of selecting pulsars to be displayed via logical conditions on parameter expressions. The web interface has an ``expert'' mode giving access to a wider range of parameters and allowing the use of custom databases. For users with locally installed software and database on unix or linux systems, the catalog may be accessed from a command-line interface. C-language functions to access specified parameters are also available. The catalog is updated from time to time to include new information.
Forward citations
Cited by 42 Pith papers
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Detection of X-ray Emission from a Bright Long-Period Radio Transient
A bright long-period radio transient shows periodic X-ray emission at the same 44.2-minute period, making it the first LPT detected in X-rays and establishing a new class of hour-scale periodic X-ray transients.
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An Acceleration is Worth a Hundred Thousand Phase Space Measurements
One acceleration measurement equals ~10^5 phase-space measurements for local dark matter density estimation, with acceleration outperforming Jeans modeling in both equilibrium and perturbed Milky Way simulations.
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A catalogue of TeV pulsar environments
A homogenized catalogue of 128 TeV sources linked to 66 pulsars shows weak correlation between TeV luminosity and pulsar age, indicating environmental effects dominate evolution.
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Timing and statistical analysis of single-pulse search pulsar discoveries from the PALFA survey
Timing solutions for five PALFA rotating radio transients, spin periods for two more, and Bayesian energy and wait-time fits that support log-normal burst energies and near-Poisson burst times.
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Relativistic effects of PSR~J1856--0039 double neutron star system in a 2.36-hour compact orbit
PSR J1856–0039 is a compact double neutron star with the lowest known total mass (2.4884 solar masses), and its orbital decay matches general relativity.
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Accurate Extragalactic Magnetic Fields from Faraday Rotation with Optimal Dispersion Measure Estimators
Calibrated on MHD galaxy simulations, an EM-based power-law estimator converts Faraday rotation measures to magnetic field strengths with ~0.1 dex error.
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Search for continuous gravitational waves from the pulsar J0435+3233
A LIGO O4a search for continuous gravitational waves from millisecond pulsar J0435+3233 finds no signal, setting h0<5.8×10^-27 at 95% confidence and an ellipticity limit of 1.6×10^-8.
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A cosmic-ray loaded nascent outflow driven by a massive star cluster
Fermi-LAT detects an extended GeV gamma-ray source and an H I cavity near Westerlund 1, interpreted as a cosmic-ray-loaded outflow leaving the Galactic disc.
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The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars
Atlas of 205 non-recycled southern pulsars at 140–170 MHz from MWA SMART data, with profiles, DMs, RMs, fluxes and public data products for SKA-Low.
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Crust glass formation reveals the neutron star birth properties in IGR J17480-2446
Accretion-induced failure of the neutron star crystal crust produces a glass layer that explains the observed cooling, fixes the accreted mass at 2.4e-6 solar masses, and indicates birth properties typical of recycled...
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Guitar Nebula: extreme accelerator in extreme environment
The Guitar nebula's pulsar appears to accelerate electrons to within ~3/4 of the theoretical maximum potential, and its brightness is best explained by the pulsar crossing an old supernova remnant's compressed, magnet...
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Stellar Superradiance and Low-Energy Absorption in Dense Nuclear Media
Collective nucleon scattering in neutron-star matter suppresses the effective absorption of ultralight bosons at the long wavelengths relevant for superradiance, weakening the link between stellar cooling bounds and s...
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A Self-Consistent Model of Kinetic Alfven Solitons in Pulsar Wind Plasma: Linking Soliton Characteristics to Pulsar Observables
Soliton width in a KdV model of pulsar-wind kinetic Alfvén waves is claimed to scale with pulsar observables, with slower pulsars hosting broader solitons.
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PHECT: A lightweight computation tool for pulsar halo emission
PHECT is a configurable computation tool for pulsar halo gamma-ray emission using multiple transport models and stable finite-volume discretizations.
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Empirical Modeling of Magnetic Braking in Millisecond Pulsars to Measure the Local Dark Matter Density and Effects of Orbiting Satellite Galaxies
A spin-down based empirical model for magnetic braking doubles the sample of pulsar acceleration measurements and yields a direct local dark matter density of 0.0098 +/- 0.0025 solar masses per cubic parsec.
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Evidences of low-diffusion bubbles around Galactic pulsars
A sample of 27 Galactic pulsar wind nebulae shows a diffusion coefficient about two orders of magnitude below the Galactic average, implying large low-diffusion bubbles around these pulsars.
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Tentative detection of circularly polarized bursty radio emissions from the HD 189733 exoplanetary system using NenuFAR beamformed observations
NenuFAR beamformed Stokes-V data tentatively show a ~10σ left-hand circularly polarized burst from HD 189733 at 27–40 MHz lasting ~16 min, offset by ~1 h from the imaging burst of Zhang et al. (2025).
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A Square Kilometre Array Pulsar Census
Composite SKA-Low + Mid Band 1/2 all-sky surveys with AA* yield ~10k slow pulsars and ~800 MSPs; AA4 yields ~20% more, rising to ~1300 MSPs if Mid coverage is broadened.
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The G347.3-0.5 outlier from O3: a follow-up case study for continuous gravitational-wave candidates
Multi-pipeline follow-up recovers the G347.3-0.5 outlier in O3 data but finds no standard persistent continuous-wave signal in O4a or O4b, disfavouring the astrophysical interpretation under the assumed model.
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Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region
Modeling favors a lepto-hadronic supernova remnant for the extended TeV emission from HESS J1834-087 plus a leptonic magnetar wind nebula for the central point-like source, with an implied magnetar birth spin period b...
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Dependences of radio pulsar parameters on the bimodal kick mode
Pulsars that received weak natal kicks tend to have weaker magnetic fields, and no fast-kicked pulsar with a field below ~10^11 G appears in the sample.
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A Log-Uniform Initial Magnetic Field Distribution Explains Pulsar and Magnetar Populations through Magnetic Inclination Alignment
Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
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Spectral energy-loss bump and $\gamma$-ray pulsar halos
The curved spectrum of the young pulsar halo LHAASO J0248+6021 is explained by a time-dependent energy-loss bump in the electron spectrum that remains close to the cutoff, unifying it with the shifted bump observed in...
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Detecting the Axion-Photon Conversion Background
Neutron star magnetospheres across the Milky Way produce a faint but statistically detectable axion-photon conversion radio background, while interstellar medium signals are too weak for current instruments.
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GeV-TeV Connections in Galaxies: Evolutionary Signatures from Pulsars in Globular Clusters
Globular cluster pulsar winds may make a significant contribution to GeV and TeV gamma-ray emission from massive quiescent galaxies, with strength tied to each galaxy's evolutionary history.
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Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo
A two-zone diffusion model fitted to HAWC morphology and spectrum data constrains Geminga's slow-diffusion zone to 30-70 pc and injection index p ≤ 2.17, reproducing AMS-02 positrons as a derived outcome.
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Constraining Axion Mass through Gamma-ray Observations of Pulsars
Under a thermally optimistic 20 MeV core model, nine years of Fermi data on 17 dark pulsars set an axion mass upper limit of 9.6e-3 eV, but realistic cooler cores suppress the signal to undetectability.
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Constraining light fermionic dark matter with binary pulsars
Dynamical friction from a degenerate fermionic dark matter background induces measurable secular decay in binary pulsar orbital periods, with sensitivity to fermion masses ≳50 eV and example upper bounds around 1 keV ...
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Astrophysical origins of TeV features in the cosmic-ray lepton spectrum
Pulsar and supernova-remnant models yield TeV electron features with effective sharpness beta_eff of roughly 2 to 3.6, so a sharper, stable edge would favor exotic origins.
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The Lunar Farside Transients and Technology Telescope (LFT3) Mission
Proposes a $150M-class lunar farside radio telescope (LFT3) to survey 0.1–2700 MHz in the RFI-pristine shielded zone before lunar-orbital interference closes the window.
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Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031
Both leptonic and lepto-hadronic models fit the CTB 37B gamma-ray spectrum; neutral-pion decay matches above ~10 TeV but needs ~10^51 erg in protons unless the remnant hits dense gas.
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SPICE: Scintillation Pipeline for Interferometric Candidate Extraction
SPICE is an automated pipeline that recovers known pulsars in GMRT data by detecting scintillation signatures in interferometric visibilities.
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The impact of FRB dispersion measure probability distribution functions on cosmographic estimates
Cosmographic constraints from 106 FRBs on H0, q0, j0 depend sensitively on whether a Gaussian or quasi-Gaussian PDF is assumed for DM_IGM and on whether the baryon mass fraction is fixed or free.
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Axial $w$-modes of anisotropic neutron stars
Axial w-mode frequencies of anisotropic neutron stars decrease monotonically with mass, depend approximately linearly on compactness with anisotropy modifying slope and intercept, damping times increase with mass, and...
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Can accreting isolated neutron stars be detected?
Updated population synthesis shows that accreting isolated neutron stars may number up to a few thousand in eROSITA data under favorable propeller-stage and accretion assumptions, though uncertainties can reduce the c...
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Fundamental Noise and Gravitational-Wave Sensitivity of the Laser Interferometer Lunar Antenna (LILA)
The Moon's normal-mode resonances would amplify gravitational-wave signals enough for the proposed LILA interferometer to reach astrophysically useful sensitivity from millihertz to decihertz.
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Understanding the Neutron Star Population with the SKAO Telescopes
SKAO AA* and AA4 surveys are projected to discover thousands of ordinary pulsars and ~800–1000 MSPs, enabling population synthesis, mass measurements and tests of gravity and emission physics.
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Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO
SKAO's sensitivity, surveys and sub-arraying will deliver tighter NS mass, MoI, spin, glitch and precession constraints that, with X-ray and GW data, probe cold ultra-dense matter.
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TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane
Alternative ISRF models produce only modest changes to the LHAASO diffuse gamma-ray fit; the associated pp neutrinos remain consistent with IceCube all-sky data and compatible with ANTARES/KM3NeT limits.
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Unlocking the hidden potential of pulsar astronomy
This review and feasibility study shows that compact radio receivers can detect bright pulsars for navigation, timing, randomness, and space weather applications, with a 4-meter dish potentially achieving 10 km self-l...
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A series of unfortunate events: CHIME/FRB misclassification of a Galactic pulsar as a periodic fast radio burst
A reported periodic fast radio burst is reclassified as Galactic pulsar emission due to CHIME calibration and beam-pointing error.
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The magnetic field of the Milky Way: an observational perspective
Review summarizing observational data on the Milky Way's magnetic field structure, including spiral alignment, halo components, turbulence, and correlations with interstellar gas and dust.
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