The Energy-dependent γ-Ray Morphology of the Crab Nebula Observed with the Fermi Large Area Telescope
Author:
Funder
DFG
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab107a/pdf
Reference26 articles.
1. THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS
2. The Search for Spatial Extension in High-latitude Sources Detected by the Fermi Large Area Telescope
3. The Crab Nebula and Pulsar between 500 GeV and 80 TeV: Observations with the HEGRA Stereoscopic Air Cerenkov Telescopes
4. Teraelectronvolt pulsed emission from the Crab Pulsar detected by MAGIC
5. On the mechanisms of gamma radiation in the Crab Nebula
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1. Spectrum and extension of the inverse-Compton emission of the Crab Nebula from a combined Fermi-LAT and H.E.S.S. analysis;Astronomy & Astrophysics;2024-06
2. Analysis of the structural complexity of Crab Nebula observed at radio frequency using a multifractal approach;Journal of Physics: Complexity;2024-01-29
3. Phenomenological modelling of the Crab Nebula’s broadband energy spectrum and its apparent extension;Astronomy & Astrophysics;2023-03
4. Multiband Emission up to PeV Energy from the Crab Nebula in a Spatially Dependent Lepto-hadronic Model;The Astrophysical Journal;2022-02-01
5. Erratum: “The Energy-dependent γ-Ray Morphology of the Crab Nebula Observed with the Fermi Large Area Telescope” (2019, ApJ, 875, 123);The Astrophysical Journal;2021-03-01
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