Fermi Large Area Telescope Performance After 10 Years Of Operation
arXiv:2106.12203 · doi:10.3847/1538-4365/ac0ceb
Abstract
The Large Area Telescope (LAT), the primary instrument for the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from 30 MeV to more than 300 GeV. We describe the performance of the instrument at the 10-year milestone. LAT performance remains well within the specifications defined during the planning phase, validating the design choices and supporting the compelling case to extend the duration of the Fermi mission. The details provided here will be useful when designing the next generation of high-energy gamma-ray observatories.
60 pages, 28 figures. Published in ApJS
References in corpus (4)
Cited by in corpus (33)
- The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
- GeV emission from a compact binary merger
- A Gamma-ray Pulsar Timing Array Constrains the Nanohertz Gravitational Wave Background
- Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring Episode
- Gamma-ray Eclipses and Orbital Modulation Transitions in the Candidate Redback 4FGL J1702.7-5655
- A magnetised Galactic halo from inner Galaxy outflows
- Ultra-High-Energy Gamma-Ray Astronomy
- Singular Spectrum Analysis of Fermi-LAT Blazar Light Curves: A Systematic Search for Periodicity and Trends in the Time Domain
- Hunting for gamma-ray emission from Fast Radio Bursts
- Classification of the \emph{Fermi}-LAT Blazar Candidates of Uncertain type using eXtreme Gradient Boosting
- Multiwavelength observations of PSR J2021+4026 across a mode change reveal a phase shift in its X-ray emission
- Fermi Gamma-ray Space Telescope
- Probing axion-like particles with multimessenger observations of neutron star mergers
- Compton Telescopes for Gamma-ray Astrophysics
- Revisiting X-ray Afterglows of Jetted Tidal Disruption Events with the External Reverse Shock
- Multi-frequency test of dark matter annihilation into long-lived particles in Sirius
- PSF Calibration of DAMPE for gamma-ray Observations
- Optical observations of the Galactic SNR HB9 and H II region G159.2+3.3
- Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
- Galaxy-cluster-stacked Fermi-LAT II: extended central hadronic signal
- Exploring non-thermal emission from the star-forming region NGC 3603 through a realistic modelling of its environment
- The Fermi Large Area Telescope
- The expected potential of hadronic PeVatron searches with spectral -ray data from the Southern Wide-field Gamma-ray Observatory
- Gamma-ray Pulsar Emission is Mostly Stable on Timescales from Minutes to Years
- Broadband Spectro-temporal Study on Blazar TXS 1700+685
- The calibrations of DAMPE -ray effective area
- Timing Gamma-ray Pulsars using Gibbs Sampling
- New high-precision measurement system for electron-positron pairs from sub-GeV/GeV gamma-rays in the emulsion telescope
- Limits on the non-thermal emission of the WR-WR system Apep
- Unveiling extended gamma-ray emission around HESS J1813-178
- Pair Production Detectors for Gamma-ray Astrophysics
- Fermi-LAT View on Three Ultra-high-energy 1LHAASO Sources in the Region
- A blind search for intraday gamma-ray transients with Fermi-LAT: Detections of GRB and solar emissions