activity
19972025
most citedThe Large Observatory for X-ray Timing (LOFT)

214 citations · 370 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2025★ 1 cited

Closing the gap: Follow-up observations of peculiar dusty objects close to Sgr A* using ERIS

F. Peißker, M. Zajacek, V. Karas +8

Context. In addition to the supermassive black hole Sgr A*, the inner parsec of our Galactic center is home to numerous fruitful scientific habitats. One of these environments is t…

astro-ph.HE2025

Constraining the TeV gamma-ray emission of SN 2024bch, a possible type IIn-L from a red supergiant progenitor. Multiwavelength observations and analysis of the progenitor

The CTAO-LST Project, :, K. Abe +332

We present very high-energy optical photometry and spectroscopic observations of SN 2024bch in the nearby galaxy NGC 3206 (\sim 20 Mpc). We used gamma-ray observations performed wi…

astro-ph.HE2025

Hybrid concept of detection for a wide-field gamma-ray observatory using Cherenkov telescopes

Alena Bakalová, Ruben Conceição, Lucio Gibilisco +6

The hybrid detection approach in astroparticle physics has been successfully employed in cosmic-ray experiments and is currently being explored by gamma-ray observatories like LHAA…

astro-ph.HE2022★ 40 cited

X-ray polarization detection of Cassiopeia A with IXPE

Jacco Vink, Dmitry Prokhorov, Riccardo Ferrazzoli +92

We report on a detection of polarized 3-6 keV X-ray emission from the supernova remnant Cassiopeia A with the Imaging X-ray Polarimetry Explorer (IXPE). The overall polar…

astro-ph.IM2021★ 9 cited

Status and results of the prototype LST of CTA

Daniel Mazin

The Large-Sized Telescopes (LSTs) of Cherenkov Telescope Array (CTA) are designed for gamma-ray studies focusing on low energy threshold, high flux sensitivity, rapid telescope rep…

astro-ph.IM2021★ 5 cited

Camera Calibration of the CTA-LST prototype

Yukiho Kobayashi, Akira Okumura, Franca Cassol +5

The Cherenkov Telescope Array (CTA) is the next-generation gamma-ray observatory that is expected to reach one order of magnitude better sensitivity than that of current telescope…