The main goal of the JEM-EUSO experiment is the study of Ultra High Energy Cosmic Rays (UHECR, 1019-1021 e V), but the method which will be used (detection of...
Search and analysis of giant radio galaxies with associated nuclei (SAGAN): V. Study of giant double-double radio galaxies from LoTSS DR2
To test the hypothesis that megaparsec-scale giant radio galaxies (GRGs) experience multiple epochs of recurrent activity leading to their giant sizes and to...
Search for low mass vector resonances decaying into quark-antiquark pairs in proton-proton collisions at √{s}=13 TeV
A search for narrow vector resonances decaying into quark-antiquark pairs is presented. The analysis is based on data collected in proton-proton collisions at √...
Search for narrow and broad dijet resonances in proton-proton collisions at √{s}=13 TeV and constraints on dark matter mediators and other new particles
Searches for resonances decaying into pairs of jets are performed using proton-proton collision data collected at √{s}=13 TeV corresponding to an integrated...
Search for top squark pair production in compressed-mass-spectrum scenarios in proton-proton collisions at √{ s} = 8 TeV using the αT variable
An inclusive search is performed for supersymmetry in final states containing jets and an apparent imbalance in transverse momentum, p→Tmiss, due to the...
Searching for the Signatures of Jet-ISM Interactions in X-ray Binaries
Jets from X-ray binaries are continuously injecting matter and energy into the surrounding interstellar medium. However, there exist to date relatively few...
Simultaneous Multiwavelength Observation of Mkn 501 in a Low State in 2006
We present results of the multiwavelength campaign on the TeV blazar Mkn 501 performed in 2006 July, including MAGIC for the very-high-energy (VHE) γ-ray band...
Simultaneous Multiwavelength Observations of the Blazar 1ES 1959+650 at a Low TeV Flux
We present the results from a multiwavelength campaign on the TeV blazar 1ES 1959+650, performed in 2006 May. Data from the optical, UV, soft- and hard-X-ray...
Coronal lines are forbidden emission lines with a ionisation potential χ ≳ 100 eV. They are linked to energetic phenomena triggered by active galactic nuclei...