The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
arXiv:2307.11132 · doi:10.3847/1538-4357/acee67
Abstract
We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of LAT sources will likely reveal pulsations once phase-connected rotation ephemerides are achieved. A further dozen optical and/or X-ray binary systems co-located with LAT sources also likely harbor gamma-ray MSPs. This catalog thus reports roughly 340 gamma-ray pulsars and candidates, 10% of all known pulsars, compared to known before Fermi. Half of the gamma-ray pulsars are young. Of these, the half that are undetected in radio have a broader Galactic latitude distribution than the young radio-loud pulsars. The others are MSPs, with 6 undetected in radio. Overall, >235 are bright enough above 50 MeV to fit the pulse profile, the energy spectrum, or both. For the common two-peaked profiles, the gamma-ray peak closest to the magnetic pole crossing generally has a softer spectrum. The spectral energy distributions tend to narrow as the spindown power decreases to its observed minimum near erg s, approaching the shape for synchrotron radiation from monoenergetic electrons. We calculate gamma-ray luminosities when distances are available. Our all-sky gamma-ray sensitivity map is useful for population syntheses. The electronic catalog version provides gamma-ray pulsar ephemerides, properties and fit results to guide and be compared with modeling results.
arXiv comment142 pages. Accepted by the Astrophysical Journal Supplement
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- Identification of radio and gamma-ray pulsars in X-rays using data from the SRG/eROSITA all-sky survey
- The Effect of Pulsar Geometry on the Observed Gamma-ray Spectrum of Millisecond Pulsars
- Probing the emission mechanism and nature of the pulsating compact object in the X-ray binary SAX J1324.4-6200
- Gamma-Ray Millisecond Pulsars: Off-pulse Emission Characteristics, Phase-Resolved Pseudo-Luminosity--Cutoff Energy Correlation, and High-energy Pulsed Emission
- Evidence for optical pulsations from a redback millisecond pulsar
- Deeper analysis of Fermi-LAT unassociated 4FGL J2112.5-3043 for possible identification
- A newly born spider system at the core of a radio shell: Evidence for a low-energy supernova
- Multi-wavelength emission in resistive pulsar magnetospheres
- No Measurable Changes in Radio and X-ray Emission Surrounding Glitches in the Young Pulsar PSR J2229+6114
- Fermi-LAT View on Three Ultra-high-energy 1LHAASO Sources in the Region