In this talk, I will overview the recent studies of LHAASO in TeV-PeV gamma-ray astronomy, including our measurements on supernova remnants, pulsar wind nebulae, massive star clusters, microquasars, and diffuse emission from the Galactic Plane.
some text
The proportional counters developed and operated by the GRAPES-3 experiment (Gamma Ray Astronomy PeV EnergieS Phase-3), Ooty, are gas-based detectors designed using mild steel rectangular tubes. The existing muon telescope of GRAPES-3, consisting of 3712 PRCs, has been in operation for the past few decades and data gathered by it has ensured the study of solar, atmospheric and cosmic muons....
The Baikal-GVD Neutrino Telescope is a cubic-kilometer scale detector being constructed in Lake Baikal. As of summer 2025, the telescope array consists of 14 clusters, including in total more than 4000 optical modules. The achievement by Baikal-GVD of the nominal sensitive volume for high-energy cascade detection of 1 km3 is expected by 2028. In this report we present the status of the...
Currently, the TAIGA-1 complex includes 4 Imaging Atmospheric Cherenkov Telescopes (IACT) of the TAIGA-IACT facility, 295 wide-angle Cherenkov detectors of the TAIGA-HiSCORE and Tunka-133 arrays, distributed over an area of 3 km^2, and 19 scintillation stations of the Tunka-Grande installation. With their help, a large volume of experimental data has already been obtained on the cosmic rays...
The Yakutsk EAS Array, one of the world's longest-running cosmic ray observatories, has undergone major modernization (2019–2021) to enhance its detection capabilities. Currently operating an upgraded hybrid system of scintillation and muon detectors, it provides precise measurements of extensive air showers in the 10¹⁶–10²⁰ eV range. Recent results include mass composition studies and...
The report reviews the current state of research at the multifunctional detector complex of the Tien Shan high-mountain scientific station of the Lebedev Physical Institute. The results of the search for new phenomena in the field of cosmic ray astrophysics, high-energy atmospheric physics, and geophysics are presented. In the field of cosmic ray astrophysics, the main results include the...
В докладе рассматривается современное состояние и перспективы развития уникального комплекса установок Баксанской нейтринной обсерватории ИЯИ РАН, состоящего из ливневых установок “Ковер-3” и “Андырчи”, и Баксанского подземного сцинтилляционного телескопа (БПСТ), для проведения исследований астрофизических источников космического излучения сверхвысоких энергий.
Одной из основных задач...
The accumulated problems of the high- and ultra-high energy cosmic ray physics and the tasks of the multichannel astronomy require the development of new experimental methods ensuring reliable identification of both primary and secondary cosmic ray particles.
To conduct breakthrough research in this area, the complex installations containing detectors of various types for multicomponent...
The Baikal-GVD Neutrino Telescope is a cubic-kilometer scale detector being constructed in Lake Baikal. The achievement by Baikal-GVD of the nominal sensitive volume for high-energy cascade detection of 1 km3 is expected by 2028. Currently, the Baikal collaboration is working on the development of a conceptual project of neutrino telescope in Lake Baikal with a volume about an order of...
Астрофизический комплекс TAIGA-100, площадью 100 км2 , создается для проведения исследований в области гамма-астрономии ПэВных энергий и космических лучей сверхвысоких энергий. В докладе будет представлена научная программа проекта, базовые детекторы и программа развертывания астрофизического комплекса.
One of the most challenging tasks in modern astrophysics is determining the nature and origin of cosmic rays with energies exceeding the Greisen-Zatsepin-Kuzmin (GZK) cutoff (~50 EeV), known as ultra-high-energy cosmic rays (UHECRs). The primary difficulty lies in their extremely low flux, necessitating experiments with vast exposure areas. The two largest ground-based observatories–the Pierre...