713 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR8 papers
- University of OxfordGB8 papers
- Friedrich-Alexander-Universität Erlangen-NürnbergDE7 papers
- Université Paris CitéFR7 papers
- Heidelberg UniversityDE6 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR6 papers
- Karlsruhe Institute of TechnologyDE6 papers
- Laboratoire de Physique Nucléaire et de Hautes ÉnergiesFR6 papers
- Max Planck Institute for Nuclear PhysicsDE6 papers
- National Institute for Subatomic PhysicsNL6 papers
- Sorbonne UniversitéFR6 papers
- The University of AdelaideAU6 papers
38 papers
Magnetic field strengths of hot giant exoplanets consistent with Solar System values
Julia V. Seidel, Vivien Parmentier, Bibiana Prinoth +29
Magnetic fields are ubiquitous in the universe. They play a key role in shaping the activity of stars, the habitability of rocky planets, and the long-term retention of planetary a…
Broadband Multi-wavelength Properties of M87 during the 2018 EHT Campaign including a Very High Energy Flaring Episode
J. C. Algaba, M. Balokovic, S. Chandra +738
The nearby elliptical galaxy M87 contains one of the only two supermassive black holes whose emission surrounding the event horizon has been imaged by the Event Horizon Telescope (…
Discovery of a Radiation Component from the Vela Pulsar Reaching 20 Teraelectronvolts
The H. E. S. S. Collaboration, :, F. Aharonian +178
Gamma-ray observations have established energetic isolated pulsars as outstanding particle accelerators and antimatter factories in the Galaxy. There is, however, no consensus rega…
Study of a pulsar wind nebula candidate around the intermediate-age pulsar PSR J1413-6205 with H.E.S.S
P. Chambéry, Y. Gallant, A. Jardin-Blicq +5
Very-high-energy -ray emission provides constraints on the morphology and the physics mechanisms involved in the evolution of pulsar wind nebulae (PWNe). In the Galactic plane,…
Performance of the MALTA Telescope
Milou van Rijnbach, Giuliano Gustavino, Phil Allport +27
MALTA is part of the Depleted Monolithic Active Pixel sensors designed in Tower 180nm CMOS imaging technology. A custom telescope with six MALTA planes has been developed for test…
Timing performance of radiation hard MALTA monolithic Pixel sensors
G. Gustavino, P. Allport, I. Asensi +26
The MALTA family of Depleted Monolithic Active Pixel Sensor (DMAPS) produced in Tower 180 nm CMOS technology targets radiation hard applications for the HL-LHC and beyond. Several…
Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy
R. López-Coto, E. de Oña Wilhelmi, F. Aharonian +2
Pulsars are factories of relativistic electrons and positrons that propagate away from the pulsar, permeating later our Galaxy. The acceleration and propagation of these particles…
Search for Quantum Gravity Using Astrophysical Neutrino Flavour with IceCube
R. Abbasi, M. Ackermann, J. Adams +378
Along their long propagation from production to detection, neutrino states undergo quantum interference which converts their types, or flavours. High-energy astrophysical neutrinos…
Multi-messenger-Athena Synergy White Paper
L. Piro, M. Ahlers, A. Coleiro +30
In this paper we explore the scientific synergies between Athena and some of the key multi-messenger facilities that should be operative concurrently with Athena. These facilities…
Detection of a particle shower at the Glashow resonance with IceCube
IceCube Collaboration, M. G. Aartsen, R. Abbasi +382
The Glashow resonance describes the resonant formation of a boson during the interaction of a high-energy electron antineutrino with an electron, peaking at an antineutrino e…
The Effect of Mission Duration on LISA Science Objectives
Pau Amaro Seoane, Manuel Arca Sedda, Stanislav Babak +38
The science objectives of the LISA mission have been defined under the implicit assumption of a 4 yr continuous data stream. Based on the performance of LISA Pathfinder, it is now…
LION :Laser Interferometer On the mooN
Pau Amaro-Seoane, Lea Bischof, Jonathan J. Carter +2
Gravitational wave astronomy has now left its infancy and has become an important tool for probing the most violent phenomena in our universe. The LIGO/Virgo-KAGRA collaboration op…
Demonstration of stellar intensity interferometry with the four VERITAS telescopes
A. U. Abeysekara, W. Benbow, A. Brill +52
High angular resolution observations at optical wavelengths provide valuable insights in stellar astrophysics, directly measuring fundamental stellar parameters, and probing stella…
Resolving acceleration to very high energies along the Jet of Centaurus A
The H. E. S. S. Collaboration, :, H. Abdalla +224
The nearby radio galaxy Centaurus A belongs to a class of Active Galaxies that are very luminous at radio wavelengths. The majority of these galaxies show collimated relativistic o…
The initial stage of cloud lightning imaged in high-resolution
O. Scholten, B. M. Hare, J. Dwyer +21
With LOFAR we have been able to image the development of lightning flashes with meter-scale accuracy and unprecedented detail. We discuss the primary steps behind our most recent l…
A very-high-energy component deep in the Gamma-ray Burst afterglow
H. Abdalla R. Adam F. Aharonian F. Ait Benkhali E. O. Anguener M. Arakawa, C. Arcaro, C. Armand +219
Gamma-ray bursts (GRBs) are brief flashes of gamma rays, considered to be the most energetic explosive phenomena in the Universe. The emission from GRBs comprises a short (typicall…
Direct measurement of stellar angular diameters by the VERITAS Cherenkov Telescopes
W. Benbow, R. Bird, A. Brill +54
The angular size of a star is a critical factor in determining its basic properties. Direct measurement of stellar angular diameters is difficult: at interstellar distances stars a…
Tunka Advanced Instrument for cosmic rays and Gamma Astronomy
D. Kostunin, I. Astapov, P. Bezyazeekov +79
The paper is a script of a lecture given at the ISAPP-Baikal summer school in 2018. The lecture gives an overview of the Tunka Advanced Instrument for cosmic rays and Gamma Astrono…
Nucleon observables and axial charges of other baryons using twisted mass fermions
Constantia Alexandrou, Martha Constantinou, Kyriakos Hadjiyiannakou +3
We present results on the nucleon scalar, axial and tensor charges, as well as, on the first moments of the unpolarized, polarized and transversity parton distributions using $N_f=…
Sigma-terms and axial charges for hyperons and charmed baryons
C. Alexandrou, K. Hadjiyiannakou, K. Jansen +1
We present results for the -terms and axial charges for various hyperons and charmed baryons using twisted mass fermions. For the computation of the three-point func…
Progress on double-logarithmic large-x and small-x resummations for (semi-)inclusive hard processes
A. Vogt, C. H. Kom, N. A. Lo Presti +5
Over the past few years considerable progress has been made on the resummation of double-logarithmically enhanced threshold (large-x) and high-energy (small-x) higher-order contrib…
Generalized threshold resummation for semi-inclusive e+e- annihilation
N. A. Lo Presti, A. Vogt, A. A. Almasy
Recently methods have been developed to extend the resummation of large-x double logarithms in inclusive deep-inelastic scattering (DIS) to terms not addressed by the soft-gluon ex…
Nucleon Structure in Lattice QCD using twisted mass fermions
C. Alexandrou, M. Constantinou, T Korzec +5
We present results on the nucleon form factors and moments of generalized parton distributions obtained within the twisted mass formulation of lattice QCD. We include a discussion…
Forward Instrumentation for ILC Detectors
Halina Abramowicz, Angel Abusleme, Konstantin Afanaciev +55
Two special calorimeters are foreseen for the instrumentation of the very forward region of the ILC detector, a luminometer designed to measure the rate of low angle Bhabha scatter…