FERMI LARGE AREA TELESCOPE FIRST SOURCE CATALOG

By A. Abdo, M. Ackermann, M. Ajello, A. Allafort, E. Antolini, W. Atwood, M. Axelsson, L. Baldini, J. Ballet, G. Barbiellini and 225 more. 2010

1,044 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/8d7e0bf25bfd13bc482712941d92bf3f40519aa9

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Nuclear and High Energy Physics

Citations in the corpus

OBSERVATIONS OF THE YOUNG SUPERNOVA REMNANT RX J1713.7−3946 WITH THE FERMI LARGE AREA TELESCOPE (2011, background): “In particular, X-ray and TeV gamma-ray43 observations of young SNRs such as Cas A (Hwang et al. 2004; Gotthelf et al. 2001; Albert44 et al. 2007; Abdo et al. 2010b), or RX J1713.”
A population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope (2010, methodology): “In addition to the diffuse components, we included all point sources (except for the source that corresponds to the globular cluster of interest) from the first-year catalogue (Abdo et al. 2010b) that were detected with TS ≥ 25 for a given ROI in the background model.”
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).”
THE LUMINOSITY FUNCTION OF FERMI-DETECTED FLAT-SPECTRUM RADIO QUASARS (2011, methodology): “This is done in order to reproduce the inherent systematic uncertainty of ﬁtting the curved spectrum of a source with a power law (Abdo et al. 2010a).”
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…”
DISCOVERY OF TeV GAMMA-RAY EMISSION FROM TYCHO’S SUPERNOVA REMNANT (2011, background): “In the GeV regime, the source does not appear in either the first Fermi LAT catalog (Abdo et al. 2010) or the 3rd EGRET catalog (Hartman et al. 1999).”
The intergalactic magnetic field constrained by Fermi/LAT observations of the TeV blazar 1ES 0229+200 (2010, background): “Following Abdo et al. (2010a), upper limits have been calculated looking at the flux satisfying2∆ log(L) = 4 when increasing the flux from the value minimizing the likelihoodL.”
A simplified view of blazars: clearing the fog around long‐standing selection effects (2011, methodology): “…far ⋆ E-mail: paolo.giommi@asdc.asi.it about 3,000 blazars are known (Massaro et al. 2009, 2011), but their number is steadily growing thanks to the Fermi (Abdo et al. 2010b, 2011), the optical Sloan Digital Sky Survey (SDSS: Plotkin et al. 2010), and the Planck (Planck Collaboration 2011) surveys.”
THE FERMI LARGE AREA TELESCOPE ON ORBIT: EVENT CLASSIFICATION, INSTRUMENT RESPONSE FUNCTIONS, AND CALIBRATION (2012, methodology): “For comparison the intensity of the extragalactic diffuse γ-ray emission measured by the LAT (Abdo et al. 2010f) is overlaid to demonstrate the many orders of background suppression necessary to distinguish it from particle background.”
Constraints on dark matter annihilation in clusters of galaxies with the Fermi large area telescope (2010, background): “The background point sources are drawn from the First Fermi-LAT source catalog, and the parameters of these sources are left fixed at their best-fit catalog values [19].”
CONTRIBUTION OF GAMMA-RAY-LOUD RADIO GALAXIES’ CORE EMISSIONS TO THE COSMIC MeV AND GeV GAMMA-RAY BACKGROUND RADIATION (2011, methodology): “Their average photon index at 0.1–10 GeV is ∼2.4, which is the same as that of the GeV EGRB (Abdo et al. 2010e) and blazars (Abdo et al. 2010f).”
THE THIRD CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THE FERMI LARGE AREA TELESCOPE (2015, methodology): “All the 1FGL sources, detected in 11 months of exposure, were subsequently studied with 15 months of data (Abdo et al. 2010e).”
Active galactic nuclei: what’s in a name? (2017, methodology): “This includes 415 FSRQs (all of the LSP type), 657 BL Lacs (mostly of the HSP type), and 402 blazars of uncertain type (assumed to be blazars because of their radio to γ -ray SED but with no optical spectrum yet available to classify them as FSRQs or BL Lacs).”
EVIDENCE FOR GAMMA-RAY HALOS AROUND ACTIVE GALACTIC NUCLEI AND THE FIRST MEASUREMENT OF INTERGALACTIC MAGNETIC FIELDS (2010, background): “This does not introduce any significant uncertainty of the stacked images, because the localization accuracy using gamma rays is typically much better than the size of PSF especially for hard AGN (Abdo et al. 2010b).”
A comment on the emission from the Galactic Center as seen by the Fermi telescope (2010, methodology): “To model the contribution from the point sources we include 19 sources from 11 monthsFermi catalog (Abdo et al. 2010a) falling into the selected region plus 4 additional sources described in Chernyakova et al. (2010).”
FERMI LARGE AREA TELESCOPE OBSERVATIONS OF THE SUPERNOVA REMNANT W28 (G6.4−0.1) (2010, methodology): “…Fermi have demonstrated that bright, extended gamma-ray sources coincident with middle-aged SNRs interacting with molecular clouds, such as W44 (Abdo et al. 2010a), W51C (Abdo et al. 2009), and IC 443 (Abdo et al. 2010b), exhibit spectral breaks from 9 GeV c−1 to a few tens of GeV c−1 in the…”