THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS

By A. Abdo, M. Ajello, A. Allafort, L. Baldini, J. Ballet, G. Barbiellini, M. Baring, D. Bastieri, A. Belfiore, R. Bellazzini and 201 more. 2013

537 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/0f3527c2359b76b1d6e48529b4b22b93dfa64522

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In Astronomy and Astrophysics

1. A. Spitkovsky
2. A. Strong
3. E. Orlando
4. A. Philippov
5. Anna Franckowiak
6. G. Dubus
7. B. Cerutti
8. Bing Zhang

In Nuclear and High Energy Physics

1. A. Spitkovsky
2. A. Strong
3. E. Orlando
4. Anna Franckowiak
5. A. Philippov
6. I. Grenier
7. Troy A. Porter
8. G. Dubus

Citations in the corpus

• Modelling high-energy pulsar light curves from first principles (2015, background): “The high-energy radiation from pulsars is characterized by short bright pulses modulated with the stellar rotation period (Abdo et al. 2010, 2013), which results most likely from the misalignment between the rotation axis and the magnetic axis of the star.”
• THE SPECTRUM OF ISOTROPIC DIFFUSE GAMMA-RAY EMISSION BETWEEN 100 MeV AND 820 GeV (2014, background): “However, the contributions of known high-latitude pulsars extracted from the second LAT pulsar catalog (Abdo et al. 2013) is less than 5% of the total EGB anywhere in the measured energy range, well below the level of systematic uncertainty inherent to the IGRB measurement.”
• 2FHL: THE SECOND CATALOG OF HARD FERMI-LAT SOURCES (2015, methodology): “We included 3FGL point and extended sources, the Galactic diffuse and isotropic emission, and pulsars from the second Fermi-LATpulsar catalog (Abdo et al. 2013; as well as from 3FGL) in the preliminary source model for each region.”
• The 2HWC HAWC Observatory Gamma-Ray Catalog (2017, methodology): “…are also searched in the FermiLAT catalogs: the standard 2FGL and 3FGL catalogs (Abdo et al. 2010a; Nolan et al. 2012; Acero et al. 2015), the high energy 1FHL and 2FHL catalogs (Ackermann et al. 2013, 2016), the second pulsar catalogs (Abdo et al. 2013), and the SNR catalog (Acero et al. 2016).”
• Interpretation of AMS-02 electrons and positrons data (2014, background): “3 - 2]) in agreement with the mean spectral index of the gamma-ray pulsars listed in the FERMI-LAT catalog [165].”
• Fermi Large Area Telescope Fourth Source Catalog (2019, background): “The counterpart catalogs (Table 6) include known γ-rayemitting source classes: AGNs (Ackermann et al. 2015), galaxies (Abdo et al. 2010b), pulsars (Abdo et al. 2013), PWNe (Ackermann et al. 2011c), SNRs (Acero et al. 2016b), globular clusters (GLCs; Abdo et al. 2010a), low- and high-mass X-ray…”
• The population of TeV pulsar wind nebulae in the H.E.S.S. Galactic Plane Survey (2017, background): “A pulsar releases a total amount of energy of up to 1049– 1050 erg over its lifetime, but only .10 % of this energy is emitted as pulsed electromagnetic radiation (Abdo et al. 2013).”
• 3FHL: The Third Catalog of Hard Fermi-LAT Sources (2017, background): “The Fermi-LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis.”
• THE FIRST FERMI-LAT CATALOG OF SOURCES ABOVE 10 GeV (2013, methodology): “The second Fermi LAT catalog of γ -ray pulsars (Abdo et al. 2013; hereafter referred to as 2PC), includes results for 117 γ -ray pulsars detected in 3 yr of LAT data.”
• Peering into the Dark Side: Magnesium Lines Establish a Massive Neutron Star in PSR J2215+5135 (2018, methodology): “If we used the pulsar timing reference epoch to calculate Φorb (which dates from 2009-12-21, from Abdo et al. 2013), we should include the orbital period derivative Ṗorb (not doing so would yield a propagated uncertainty to our 2014-08-02 epoch of 0.02 orbital cycles).”
• DEVELOPMENT OF THE MODEL OF GALACTIC INTERSTELLAR EMISSION FOR STANDARD POINT-SOURCE ANALYSIS OF FERMI LARGE AREA TELESCOPE DATA (2016, background): “They generally have much harder spectra than the interstellar emission (Abdo et al. 2013), but they contribute at best a few percent of the diffuse emission (see Section 2.4).”
• FERMI-LAT OBSERVATIONS OF HIGH-ENERGY γ-RAY EMISSION TOWARD THE GALACTIC CENTER (2015, background): “0.2 kpc) and are listed in the LAT Second Catalog of Gamma-ray Pulsars24 (Abdo et al. 2013).”
• Particle acceleration in axisymmetric pulsar current sheets (2014, background): “Young pulsars represent the majority of the high-energy gamma-ray sources identified in our Galaxy (Abdo et al. 2013).”