Results 21 to 30 of about 2,379,646 (229)
We present the current status of high-energy cosmic-ray physics and gamma-ray astronomy at the Tunka Astrophysical Center (AC). This complex is located in the Tunka Valley, about 50 km from Lake Baikal.
Kuzmichev L. +76 more
doaj +2 more sources
Gamma Ray Astronomy with ARGO-YBJ [PDF]
ARGO‐YBJ is the first EAS detector combining a very high mountain altitude (4300 m a.s.1.) to a “full coverage” detection surface. These features allow ARGO‐YBJ to work with an energy threshold as low as a few hundreds GeV. The high duty cycle and the large field of view (∼2 sr) make ARGO‐YBJ suitable to monitor the gamma ray sky, searching for unknown
Aielli G +110 more
openaire +3 more sources
A General Overview for Localizing Short Gamma-Ray Bursts with a CubeSat Mega-Constellation
The gamma-ray burst monitor (GBM) on the Fermi Gamma-Ray Space Telescope, for the first time, detected a short gamma ray burst (SGRB) signal that accompanies a gravitational wave signal GW170817 in 2017.
Fadil Inceoglu +5 more
doaj +1 more source
Diffuse γ -ray emission between 10 and 1000 TeV from the Galactic plane was recently measured by the Large High Altitude Air Shower Observatory (LHAASO).
Rui Zhang +4 more
doaj +1 more source
Gamma-Ray Astrophysics in the Time Domain
The last few years have seen gamma-ray astronomy maturing and advancing in the field of time-domain astronomy, utilizing source variability on timescales over many orders of magnitudes, from a decade down to a few minutes and shorter, depending on the ...
Frank M. Rieger
doaj +1 more source
Gamma-Ray Line Astronomy [PDF]
9 pages, 5 figures; invited review at "Nuclei in the Cosmos 8", Vancouver, CA; accepted for publication in Nucl Phys ...
openaire +4 more sources
AGILE Gamma-Ray Detection of the Exceptional GRB 221009A
Gamma-ray emission in the MeV–GeV range from explosive cosmic events is of invaluable relevance to understanding physical processes related to the formation of neutron stars and black holes.
Marco Tavani +49 more
doaj +1 more source
Radio and γ-ray Evidence for the Supernova Origin of High-velocity Cloud Complex M
Using λ 21 cm galactic neutral hydrogen data from the HI4PI survey and 0.75–30 MeV γ -ray emission from the Imaging Compton Telescope, we have searched for the origin event that accelerated high-velocity cloud Complex M.
J. T. Schmelz, G. L. Verschuur
doaj +1 more source
Invited review, published in Research in Astronomy and Astrophysics (see http://www.raa-journal.org/raa/index.php/raa/article/view/251)
openaire +2 more sources
A set of plots related to gamma-ray and hadron initated air showers. Note that this is a rather random selection of plots and prepared a long time ago (in 2005).
Gernot Maier
core +1 more source

