FERMI LARGE AREA TELESCOPE SECOND SOURCE CATALOG

By P. Nolan, A. Abdo, M. Ackermann, M. Ajello, A. Allafort, E. Antolini, W. Atwood, M. Axelsson, L. Baldini, J. Ballet and 227 more. 2011

1,003 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/eae40b1ff37082edaa81f582d908bf3fd235972b

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In Astronomy and Astrophysics

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Citations in the corpus

• Time-dependent 3D magnetohydrodynamic pulsar magnetospheres: oblique rotators (2012, background): “1 IN T RO D U C T I O N The launch of the Fermi satellite opened a new window into studying the properties of pulsar magnetospheres, with more than 100 γ -ray pulsars detected (Nolan et al. 2012).”
• The IceCube Realtime Alert System (2016, background): “The list of monitored sources is based on the second Fermi point-source catalog [39], containing mostly BL-Lac objects and FSRQs, which have exhibited previous variable behavior and are visible to the follow-up telescopes.”
• Galactic Searches for Dark Matter (2012, background): “ by cosmic rays. The shape and the 71 0 0.05 0.15 0.35 0.74 1.5 3.1 6.2 13 25 50 Figure 10 Two year all sky Fermi-LAT map of the energy ux. The bottom legend is the ux in units of 10 7 cm 2 s 1. From Nolan et al. (2012). orientation of the shower allows for a discrimination between those events gene”
• THE ORIGIN OF THE EXTRAGALACTIC GAMMA-RAY BACKGROUND AND IMPLICATIONS FOR DARK MATTER ANNIHILATION (2015, methodology): “At high Galactic latitudes, Fermi-LAT has detected blazars, star-forming galaxies, radio galaxies and millisecond pulsars (Abdo et al. 2010b; Nolan et al. 2012).”
• SEARCH FOR COSMIC-RAY-INDUCED GAMMA-RAY EMISSION IN GALAXY CLUSTERS (2013, background): “Note that this radius is usually smaller than R200/2. isotropic emission components as well as individual γray sources reported in the 2nd Fermi-LAT catalog (Nolan et al. 2012, 2FGL).”
• THE LUMINOSITY FUNCTION OF FERMI-DETECTED FLAT-SPECTRUM RADIO QUASARS (2011, background): “More distant sources have parameters frozen at the 2FGL measured values (Nolan et al. 2012).”
• THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS (2013, methodology): “In addition to 1PC, this catalog builds on the 2nd Fermi LAT source catalog (Nolan et al. 2012, hereafter 2FGL), which reported pulsations for 83 of the 2FGL sources, included here.”
• The 5th edition of the Roma-BZCAT. A short presentation (2015, methodology): “The Fermi-LAT collaboration, in fact, used it at this purpose in various γ-ray source catalogues, like 1FGL (Abdo et al. 2010a), 1LAC (Fermi LAT AGN Catalog, Abdo et al. 2010b) and the subsequent 2FGL (Nolan et al. 2012) and 2LAC (Ackermann et al. 2011).”
• OBSERVATION AND CHARACTERIZATION OF A COSMIC MUON NEUTRINO FLUX FROM THE NORTHERN HEMISPHERE USING SIX YEARS OF ICECUBE DATA (2016, background): “Figure 15 shows the direction of the event with its angular uncertainty and nearby high-energy gamma-ray sources from Nolan et al. (2012), Acero et al. (2015), Wakely & Horan (2007) in a window centered around the arrival direction.”
• DEVELOPMENT OF THE MODEL OF GALACTIC INTERSTELLAR EMISSION FOR STANDARD POINT-SOURCE ANALYSIS OF FERMI LARGE AREA TELESCOPE DATA (2016, methodology): “We have modeled each source with a simple disk shape, a ring, a two-dimensional (2D) Gaussian function, or a map derived from other wavelengths, as described in Nolan et al. (2012) and Ballet & Burnett (2013).”
• The 2HWC HAWC Observatory Gamma-Ray Catalog (2017, methodology): “GeV counterparts 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…”
• GeV OBSERVATIONS OF STAR-FORMING GALAXIES WITH THE FERMI LARGE AREA TELESCOPE (2012, methodology): “Each of the four gamma-ray sources is associated with the corresponding galaxy from our sample according to the 2FGL catalog (Nolan et al. 2012).”
• 2FHL: THE SECOND CATALOG OF HARD FERMI-LAT SOURCES (2015, methodology): “The approach for automated source association closely follows that used for the 2FGL, 1FHL, 3FGL and 3LAC catalogs (Nolan et al. 2012; Ackermann et al. 2013; Acero et al. 2015; Ackermann et al. 2015).”