The First Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

Abstract

The dramatic increase in the number of known gamma-ray pulsars since the launch of the Fermi Gamma-ray Space Telescope (formerly GLAST) offers the first opportunity to study a population of these high-energy objects. This catalog summarizes 46 high-confidence pulsed detections using the first six months of data taken by the Large Area Telescope (LAT), Fermi's main instrument. Sixteen previously unknown pulsars were discovered by searching for pulsed signals at the positions of bright gamma-ray sources seen with the LAT, or at the positions of objects suspected to be neutron stars based on observations at other wavelengths. Pulsed gamma-ray emission was discovered from twenty-four known pulsars by using ephemerides (timing solutions) derived from monitoring radio pulsars. Eight of these new gamma-ray pulsars are millisecond pulsars. The pulsed energy spectra can be described by a power law with an exponential cutoff, with cutoff energies in the range 1 to 5 GeV. The rotational energy loss rate (\dot{E}) of these neutron stars spans 5 decades, from ~3x10^{33} erg/s to 5x10^{38} erg/s, and the apparent efficiencies for conversion to gamma-ray emission range from ~0.1% to unity, although distance uncertainties complicate efficiency estimates. The pulse shapes show substantial diversity, but roughly 75% of the gamma-ray pulse profiles have two peaks, separated by >0.2 of rotational phase. For most of the pulsars, gamma-ray emission appears to come mainly from the outer magnetosphere, while polar-cap emission remains plausible for a remaining few. Finally, these discoveries suggest that gamma-ray-selected young pulsars are born at a rate comparable to that of their radio-selected cousins and that the birthrate of all young gamma-ray-detected pulsars is a substantial fraction of the expected Galactic supernova rate.

Astrophysical Journal Supplement 187, 460-494 (2010 April). 85 pages. Erratum corrected in this version, 2010 December (radio-gamma phase offset for PSR J1124-5916)

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• Gamma rays, electrons and positrons up to 3 TeV with the Fermi Gamma-ray Space Telescope
• Detection of X-Ray Emission from the Unidentified TeV Gamma-Ray Source TeV J2032+4130
• Impact of the orbital uncertainties on the timing of pulsars in binary systems
• High energy gamma-ray emission from compact galactic sources in the context of observations with the next generation Cherenkov Telescope Arrays
• Particle acceleration in the expanding blast wave of Eta Carina's Great Eruption of 1843
• The Dark Knight Falters
• On the Global Structure of Pulsar Force-free Magnetosphere
• VLT Suzaku observations of the Fermi pulsar PSR J1028-5819
• Discovery of an extended source of gamma-ray emission in the Southern Hemisphere
• The Extended X-ray Nebula of PSR J1420-6048
• Investigation of gamma-ray variability and glitches of PSR J1420-6048
• Radio and Gamma-Ray Constraints on the Emission Geometry and Birthplace of PSR J2043+2740
• Classification of pulsars with Dirichlet process Gaussian mixture model
• Lower bounds of altitudes for pulsar $\gamma$-ray radiation
• Is Calvera a Gamma-ray Pulsar?
• X-ray and gamma-ray orbital variability from the gamma-ray binary HESS J1832-093
• The gamma-ray spectrum of Geminga and the inverse Compton model of pulsar high energy emission
• Dynamics of ultrarelativistic charged particles with strong radiation reaction. I. Aristotelian equilibrium state
• Scaling up global kinetic models of pulsar magnetospheres using a hybrid force-free-PIC numerical approach
• Synthetic pulsar lightcurves from global kinetic simulations and comparison with the Fermi-LAT catalog
• Three-dimensional dissipative pulsar magnetospheres with Aristotelian electrodynamics
• Optical Observations of PSR J0205+6449 - the next optical pulsar?
• The White Dwarf Companion of a 2 M_sun Neutron Star
• Study of maximum electron energy of sub-PeV pulsar wind nebulae by multiwavelength modelling
• Prospects for the detection of high-energy (E>25 GeV) Fermi pulsars with the Cherenkov Telescope Array
• Discovery of a Pulsar Wind Nebula Candidate in the Cygnus Loop
• Modeling the non-recycled Fermi gamma-ray pulsar population
• Decade Long Timing Study of the Black Widow Millisecond Pulsar J1544+4937
• Broadband X-ray Spectroscopy of the Pulsar Wind Nebula in HESS J1640-465
• Gravitational Waves from Gamma-Ray Pulsar Glitches
• PSR B1133+16: radio emission height and plasma composition
• A 350-MHz Green Bank Telescope Survey of Unassociated Fermi LAT Sources: Discovery and Timing of Ten Millisecond Pulsars
• Inverse Mapping of Polarised Optical Emission from Pulsars : Basic Formulation and Determination of Emission Altitude
• Possible Distance Indicators in Gamma-ray Pulsars
• Phase-Averaged Gamma-Ray Spectra from MSPs
• Extracting the unresolved pulsar contribution to the gamma-ray background
• Search for gamma-ray emission from four accreting millisecond pulsars with Fermi/LAT
• Population study for gamma-ray pulsars; II Millisecond pulsars
• Deep optical imaging of the gamma-ray pulsar J1048-5832 with the VLT
• A Study of the Long-term Spectral Variations of 3C 66A Observed with the Fermi and Kanata Telescopes
• Emission Patterns and Light Curves of Gamma-Rays in the Pulsar Magnetosphere with a Current-Induced Magnetic Field
• Timing Offset Calibration of CZTI instrument aboard ASTROSAT
• A New Perspective on the Diffuse Gamma-Ray Emission Excess
• Pulsar Wind Nebulae and Cosmic Rays: A Bedtime Story
• Search for Very High-Energy Emission from the millisecond pulsar PSR J0218+4232
• Conservative upper limits on WIMP annihilation cross section from Fermi-LAT $\gamma$-rays
• Multi-wavelength emission region of gamma-ray emitting pulsars
• Very Hight Energy Observationa of Shell-Type Supernova Remnants with SHALON Mirror Cherenkov Telescopes
• Synchrotron Emission From Young And Nearby Pulsars
• Cosmic Ray e^+/(e^- + e^+) and pbar/p Ratios Explained by an Injection Model Based on Gamma-ray Observations
• High energy emission from the nebula around the Black Widow binary system containing millisecond pulsar B1957+20
• The mechanism of coherent radio emission in some classes of pulsar
• AGILE study of the gamma-ray emission from the SNR G78.2+2.1 (Gamma Cygni)
• MAGIC Upper Limits for two Milagro-detected, Bright Fermi Sources in the Region of SNR G65.1+0.6
• A comprehensive search for Long and Short Periodic Features from an Extremely Active Cycle of FRB 20240114A
• Beyond the 2nd Fermi Pulsar Catalog
• Pulsars in Gamma Rays: What Fermi Is Teaching Us
• Experimental Constraints on γ-ray Pulsar Gap Models and the Pulsar GeV to Pulsar Wind Nebula TeV Connection
• CANGAROO-III observation of TeV gamma rays from the unidentified gamma-ray source HESS J1614-518
• Physics of radio emission in gamma-ray pulsars
• Prediction of radio-quiet gamma-ray pulsar distances using the Fundamental Plane relation
• Detection of precessing circumpulsar disks
• On the mechanism of the pulsed high energy emission from the pulsar PSR B1509-58
• Trajectories and Radiation of Charged Particles in the Pulsar Magnetosphere
• The strange case of HESS J0632+057 and the γ-ray High Mass X-ray Binaries
• Fermi-LAT Detection of Gamma-ray Pulsars above 10 GeV
• Possible counterpart signal of the Fermi bubbles at the cosmic-ray positrons
• Classifying Unidentified Gamma-ray Sources
• Results from the binaries LS I +61°303 and LS 5039 after 2.5 years of Fermi monitoring
• Lepton Acceleration in Pulsar Wind Nebulae
• Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling
• Resonant Inverse Compton Scattering and Hard X-ray Emission in Magnetar Magnetospheres
• Gamma-Ray Millisecond Pulsars: Off-pulse Emission Characteristics, Phase-Resolved Pseudo-Luminosity--Cutoff Energy Correlation, and High-energy Pulsed Emission
• Pulsar observations with the Fermi LAT: what we have seen
• Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars
• Pulsar emission in the very-high-energy regime
• Time Evolution of Pulsar Magnetosphere I - An Implicit Approach
• Gamma-ray Emission from Millisecond Pulsars - An Outergap Perspective
• The pulsar gamma-ray emission from the high-resolution dissipative magnetospheres
• Young radio-loud gamma-ray pulsar light-curve fitting
• The Gamma-ray Sky with Fermi
• New Neighbours: Modelling the Growing Population of Gamma-ray Millisecond Pulsars
• A method for evaluating the expectation value of a power spectrum using the probability density function of phases
• Pulsar-driven Jets in Supernovae, Gamma-Ray Bursts, and the Universe
• Fermi LAT observation of VER J2019+407
• Identification of radio and gamma-ray pulsars in X-rays using data from the SRG/eROSITA all-sky survey