output
20052026
most citedSearch for dark matter annihilations towards the inner Galactic halo from 10 years of observations with H.E.S.S

314 citations

95 papers

physics.ins-det2026

Capacitively Coupled GaAs p-i-n/Substrate Photodetector with Ohmic Contacts on Lightly Doped n-GaAs for Hard X-Ray Imaging

V. G. Harutyunyan, S. D. Zilio, M. Colja +5

In this work, we present a capacitively coupled GaAs p +-i-n/substrate photodetector (CC-GaAs PIN/S PD), which also represents a preliminary step toward 3D detection (x, y, time) o…

astro-ph.HE2026★ 2 cited

Dust and Ices in the SNR

A. Yeghikyan, M. Rah, S. Shamyar

The presence of dust in supernova remnants (SNRs) is confirmed by extensive infrared data from observatories such as Spitzer, Herschel, and JWST, alongside theoretical models of du…

astro-ph.HE2026★ 3 cited

Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights

Maria Rah, Areg Mickaelian, Francesco Flammini Dotti +1

We present a statistical study of pulsars and millisecond pulsars (MSPs) based on multiwavelength observations in the Galactic Field and Globular Clusters. We examine their emissio…

math.CA2026

On UC-multipliers for multiple trigonometric systems

Grigori A. Karagulyan

We investigate the class of sequences that can serve as almost-everywhere convergence Weyl multipliers for all rearrangements of multiple trigonometric systems. We show that…

astro-ph.GA2025

Signatures of Galactic Expansion in Gaia DR3: Implications for the JWST Early-Galaxy Puzzle

G. S. Karapetian, A. P. Mahtessian, L. E. Byzalov +2

Recent observations with the James Webb Space Telescope (JWST) of massive galaxies at ages below 1 Gyr pose a challenge to standard models of galaxy formation, which predict signif…

math.PR2024★ 4 cited

Gibbs scheme in the theory of random fields

L. A. Khachatryan, B. S. Nahapetian

The purpose of this work is to expand and clarify the concept of the class of Gibbs random fields and give its structure the form accepted in the theory of random processes. It is…