Identifying the brightest Galactic globular clusters for future observations by H.E.S.S. and CTA
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/473/1/897/21383598/stx2336.pdf
Reference58 articles.
1. A population of gamma-ray emitting globular clusters seen with theFermiLarge Area Telescope
2. Very-high-energy gamma-ray emission from the direction of the Galactic globular cluster Terzan 5
3. Search for very-high-energyγ-ray emission from Galactic globular clusters with H.E.S.S.
4. MAGIC upper limits to the VHE gamma-ray flux of 3C 454.3 in high emission state
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1. Evidence for a high-energy tail in the gamma-ray spectra of globular clusters;Monthly Notices of the Royal Astronomical Society;2021-08-23
2. Cherenkov Telescope Array sensitivity to the putative millisecond pulsar population responsible for the Galactic Centre excess;Monthly Notices of the Royal Astronomical Society;2021-05-21
3. Assessing uncertainties in the predicted very high energy flux of globular clusters in the Cherenkov Telescope Array era;Monthly Notices of the Royal Astronomical Society;2020-11-19
4. Probing the Pulsar Population of Terzan 5 via Spectral Modeling;The Astrophysical Journal;2019-07-24
5. Deep observations of the globular cluster M15 with the MAGIC telescopes;Monthly Notices of the Royal Astronomical Society;2019-01-21
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