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The Cherenkov Telescope Array
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The Cherenkov Telescope Array
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The Cherenkov Telescope Array Observatory (CTAO) is a next-generation facility for ground-based very high energy gamma ray astronomy. CTAO will be operated as an open observatory. With two sites, in the northern and southern hemispheres, the Cherenkov Telescope Array CTA will provide full-sky coverage, improving sensitivity by an order of magnitude over current instruments, with a wide gamma ray energy coverage from 20 GeV to 300 TeV. CTA will use telescope arrays composed of three types of telescopes, optimized to cover different energy ranges. The large telescopes covering the lowest energies provide rapid slewing capability, for follow-up of transients. Key Science Projects (KSPs) are developed to form a significant part of the CTAO observing program during the first decade of operation, providing legacy data sets such as surveys or deep observations of key targets.
Forward citations
Cited by 10 Pith papers
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Predicting Multiwavelength Emission Associated with X-Ray Flares and Extended Emission of Gamma-Ray Bursts
A one-zone synchrotron model of GRB X-ray flares predicts UV and VHE counterparts detectable together about once every three years, separating jet dissipation radius and Lorentz factor regimes.
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Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible...
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Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
PIC-motivated acceleration in GRB afterglows produces an observable GeV synchrotron cutoff in low-density short bursts that future observations can use to distinguish from the Bohm limit.
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A MINOT-based Study of Gamma-ray emission from SPT-CL J2012-5649/Abell 3667
MINOT modeling of Abell 3667 predicts a hadronic 1–300 GeV flux of ~1.15e-10 cm^-2 s^-1 at 3.7 R500, matching Fermi-LAT, with ~76% of flux outside R500 and IC subdominant by ~20.
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Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
PIC-motivated acceleration models for GRB afterglows predict a GeV-band synchrotron cutoff in low-density short GRBs that current Fermi-LAT data cannot distinguish from the Bohm limit but future observations could.
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The Emerging Population of High-energy Emitting Radio Galaxies
Gamma-ray detections from misaligned radio galaxies support a unifying leptonic (and possibly hadronic) emission framework across AGN scales, with SKA enabling resolved studies of particle acceleration sites.
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A MINOT-based Study of Gamma-ray emission from SPT-CL J2012-5649/Abell 3667
MINOT modeling of Abell 3667 predicts hadronic gamma-ray flux roughly matching Fermi-LAT observations in the 1-300 GeV band but with a spectral index in tension with the data.
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Supernova remnants in the new radio astronomy era
A review summarizing current challenges in radio observations of supernova remnants and the expected scientific gains from SKA-era instruments.
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Probing the Fundamental Nature of Particle Dark Matter
Review summarizing radio searches for WIMP and ALP dark matter with SKA precursors and forecasts for SKA-Low and SKA-Mid telescopes.
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Pulsar Wind Nebulae (PWNe) -- A Review
A review of Pulsar Wind Nebulae that outlines recent theoretical progress on broadband spectra and spatial features while identifying remaining questions on particle acceleration.
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