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The expected very-high-energy flux from a population of globular clusters
(SAIt, 2015)
Given their old ages, globular clusters are expected to harbour many evolved
stellar objects. Their high core densities enhance stellar encounter rates, also facilitating the
formation of stellar end products. In particular, ...
The ASTRI dual-mirror small-size Cherenkov telescope
(Sissa Medialab, 2018)
The ASTRI dual-mirror small-size telescope (ASTRI-Horn) is an imaging atmospheric Cherenkov telescope that was developed by the Italian National Institute of Astrophysics (INAF) within the framework of the Cherenkov Telescope ...
Investigating the hot gas in active brightest cluster galaxies
(PoS, 2016)
We investigate a crucial phase in the cooling–feedback cycle in the star forming Brightest Clus-
ter Galaxies (BCGs) by looking at the optical emission line properties of the reheated gas that
ultimately causes the cycle ...
On the underlying particles in the jet of 3C 279
(PoS, 2017)
Recent high-energy missions have allowed keeping watch over blazars in flaring states, which
provide deep insights into the engine powered by supermassive black holes. However, having
a blazar caught in a very bright ...
Acceleration of galactic electrons at the solar wind termination shock and Voyager 1 observations
(PoS, 2017)
Diffusive shock acceleration (DSA)
,
as an acceleration
process
for
G
alactic electrons at the solar
wind termination shock (TS)
,
is investigated
with a
comprehensive
numerical model
which ...
High-energy emission properties of pulsars
(PoS, 2017)
The sheer number of new γ-ray pulsar discoveries by the Fermi Large Area Telescope since 2008,
combined with the quality of new multi-frequency data, has caused a revolution in the field of
high-energy rotation-powered ...
Monitoring of the FSRQ PKS 1510-089 with H.E.S.S.
(PoS, 2017)
The flat spectrum radio quasar (FSRQ) PKS 1510-089 (z=0.361) is known for its complex multiwavelength
behavior. It has been monitored regularly at very high energy (VHE, E > 100GeV)
gamma-rays with H.E.S.S. since its ...
The FSRQ PKS 1510-089: the gamma-ray-synchrotron connection
(PoS, 2017)
The flat spectrum radio quasar (FSRQ) PKS 1510-089 (z=0.361) is known for its complex multiwavelength
behaviour. Since 2015, it has been very active across the entire electromagnetic spectrum.
This has lead to joint ...
Short-term variation in the galactic cosmic ray intensity measured with the PAMELA experiment
(PoS, 2017)
New results on the galactic cosmic ray (GCR) short-term intensity variation associated with Forbush
decrease and co-rotating interaction regions (CIRs) measured by the PAMELA instrument
between November 2006 and March ...
Charge-sign dependent modulation of cosmic ray electrons and positrons up to extreme solar maximum conditions
(PoS, 2017)
The charge-sign dependent modulation of cosmic rays is an important topic in solar modulation
studies, providing insights into gradient, curvature, and current sheet drifts. Such studies, at
higher levels of solar activity, ...