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19992025
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 8k across the 210 of their papers we have counts for

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23 papers · 1 filter

astro-ph.IM2024

Evaluation of the X-ray SOI pixel detector with the on-chip ADC

Hiroumi Matsuhashi, Kouichi Hagino, Aya Bamba +16

XRPIX is the monolithic X-ray SOI (silicon-on-insulator) pixel detector, which has a time resolution better than 10 s as well as a high detection efficiency for X-rays above…

astro-ph.IM2023

Imaging Atmospheric Cherenkov Telescopes pointing determination using the trajectories of the stars in the field of view

Mykhailo Dalchenko, Matthieu Heller

We present a new approach to the pointing determination of Imaging Atmospheric Cherenkov Telescopes (IACTs). This method is universal and can be applied to any IACT with minor modi…

astro-ph.IM2023★ 13 cited

Performance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data

H. Abe, K. Abe, S. Abe +365

Aims. LST-1, the prototype of the Large-Sized Telescope for the upcoming Cherenkov Telescope Array Observatory, is concluding its commissioning in Observatorio del Roque de los Muc…

astro-ph.IM2023

Characterization of SiPM and development of test bench modules for the next-generation cameras for Large-Sized Telescopes for Cherenkov Telescope Array

Takayuki. Saito, K. Hashiyama, H. Iwasaki +5

The recent improvements in the performance of the silicon photomultipliers (SiPMs) made them attractive options as photo sensors of imaging atmospheric Cherenkov telescopes (IACTs)…

astro-ph.IM2022★ 10 cited

Event reconstruction of Compton telescopes using a multi-task neural network

Satoshi Takashima, Hirokazu Odaka, Hiroki Yoneda +4

We have developed a neural network model to perform event reconstruction of Compton telescopes. This model reconstructs events that consist of three or more interactions in a detec…

astro-ph.IM2022★ 1 cited

Calibration and performance of the readout system based on switched capacitor arrays for the Large-Sized Telescope of the Cherenkov Telescope Array

Seiya Nozaki, Kyosuke Awai, Aya Bamba +59

The Cherenkov Telescope Array (CTA) is the next-generation ground-based very-high-energy gamma-ray observatory. The Large-Sized Telescope (LST) of CTA is designed to detect gamma r…

astro-ph.IM2021★ 5 cited

Simulation-based spectral analysis of X-ray CCD data affected by photon pile-up

Tsubasa Tamba, Hirokazu Odaka, Aya Bamba +6

We have developed a simulation-based method of spectral analysis for pile-up affected data of X-ray CCDs without any loss of photon statistics. As effects of the photon pile-up app…

astro-ph.IM2021★ 2 cited

Cross-calibration and combined analysis of the CTA-LST prototype and the MAGIC telescopes

Y. Ohtani, A. Berti, D. Depaoli +13

The Cherenkov Telescope Array (CTA) will be the next generation gamma-ray observatory, which will consist of three kinds of telescopes of different sizes. Among those, the Large Si…

astro-ph.IM2021

Reconstruction of extensive air shower images of the first Large Size Telescope prototype of CTA using a novel likelihood technique

Gabriel Emery, Cyril Alispach, Mykhailo Dalchenko +3

Ground-based gamma-ray astronomy aims at reconstructing the energy and direction of gamma rays from the extensive air showers they initiate in the atmosphere. Imaging Atmospheric C…

astro-ph.IM2021★ 1 cited

Commissioning of the camera of the first Large Size Telescope of the Cherenkov Telescope Array

T. Saito, C. Delgado, O. Blanch +30

The first Large Size Telescope (LST-1) of the Cherenkov Telescope Array has been operational since October 2018 at La Palma, Spain. We report on the results obtained during the cam…

astro-ph.IM2021★ 1 cited

Monitoring the pointing of the prototype LST-1 using star reconstruction in the Cherenkov camera

L. Foffano, A. Carosi, M. Dalchenko +3

The first Large-Sized Telescope (LST-1) proposed for the forthcoming Cherenkov Telescope Array (CTA) has started to operate in 2019 in La Palma. The large structure of LST-1 - with…

astro-ph.IM2020

Artifact-less Coded Aperture Imaging in the X-ray Band with Multiple Different Random Patterns

Tomoaki Kasuga, Hirokazu Odaka, Kosuke Hatauchi +7

The coded aperture imaging technique is a useful method of X-ray imaging in observational astrophysics. However, the presence of imaging noise or so-called artifacts in a decoded i…

astro-ph.IM2020★ 1 cited

Development of the detector simulation framework for the Wideband Hybrid X-ray Imager onboard FORCE

Hiromasa Suzuki, Tsubasa Tamba, Hirokazu Odaka +8

FORCE is a Japan-US space-based astronomy mission for an X-ray imaging spectroscopy in an energy range of 1--80 keV. The Wideband Hybrid X-ray Imager (WHXI), which is the main foca…

astro-ph.IM2018★ 11 cited

A Technique for Estimating the Absolute Gain of a Photomultiplier Tube

M. Takahashi, Y. Inome, S. Yoshii +26

Detection of low-intensity light relies on the conversion of photons to photoelectrons, which are then multiplied and detected as an electrical signal. To measure the actual intens…

astro-ph.IM2018★ 39 cited

Soft X-ray Imager aboard Hitomi (ASTRO-H)

Takaaki Tanaka, Hiroyuki Uchida, Hiroshi Nakajima +25

The Soft X-ray Imager (SXI) is an imaging spectrometer using charge-coupled devices (CCDs) aboard the Hitomi X-ray observatory. The SXI sensor has four CCDs with an imaging area si…

astro-ph.IM2017★ 27 cited

In-orbit performance of the soft X-ray imaging system aboard Hitomi (ASTRO-H)

H. Nakajima, Y. Maeda, H. Uchida +46

We describe the in-orbit performance of the soft X-ray imaging system consisting of the Soft X-ray Telescope and the Soft X-ray Imager aboard Hitomi. Verification and calibration o…

astro-ph.IM2014★ 55 cited

The ASTRO-H X-ray Astronomy Satellite

Tadayuki Takahashi, Kazuhisa Mitsuda, Richard Kelley +250

The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions developed by the Institute of Space and Astronautical Science (ISAS), with a planne…

astro-ph.IM2013★ 4 cited

The Cherenkov Telescope Array Large Size Telescope

G. Ambrosi, Y. Awane, H. Baba +129

The two arrays of the Very High Energy gamma-ray observatory Cherenkov Telescope Array (CTA) will include four Large Size Telescopes (LSTs) each with a 23 m diameter dish and 28 m…

astro-ph.IM2013★ 6 cited

Development of the Photomultiplier-Tube Readout System for the CTA Large Size Telescope

H. Kubo, R. Paoletti, Y. Awane +51

We have developed a prototype of the photomultiplier tube (PMT) readout system for the Cherenkov Telescope Array (CTA) Large Size Telescope (LST). Two thousand PMTs along with thei…

astro-ph.IM2011★ 48 cited

Data-oriented Diagnostics of Pileup Effects on the Suzaku XIS

Shin'ya Yamada, Hideki Uchiyama, Tadayasu Dotani +11

We present the result of a systematic study of pileup phenomena seen in the X-ray Imaging Spectrometer, an X-ray CCD instrument, onboard the Suzaku observatory. Using a data set of…

astro-ph.IM2010★ 159 cited

The ASTRO-H Mission

Tadayuki Takahashi, Kazuhisa Mitsuda, Richard Kelley +174

The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will…

astro-ph.IM2010★ 902 cited

Design Concepts for the Cherenkov Telescope Array

The CTA Consortium

Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray…

astro-ph.IM2009

Modeling and Reproducibility of Suzaku HXD PIN/GSO Background

Yasushi Fukazawa, Tsunefumi Mizuno, Shin Watanabe +26

Suzaku Hard X-ray Detector (HXD) achieved the lowest background level than any other previously or currently operational missions sensitive in the energy range of 10--600 keV, by u…