activity
20132025
most citedSensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

135 citations · 671 across the 41 of their papers we have counts for

collaborators

40 papers

astro-ph.SR2025★ 1 cited

Super-slowly rotating Ap (ssrAp) stars: New spectroscopic observations

Gautier Mathys, Daniel L. Holdsworth, Marina Giarrusso +2

The rotation periods of Ap stars range over five to six orders of magnitude. The origin of their differentiation remains unknown. We carry out a systematic study of the longest per…

astro-ph.SR2025

Pulsating and Non-pulsating Components of Detached Eclipsing Binaries in the Scuti instability strip

Filiz Kahraman Aliçavuş, Fahri Aliçavuş, Zeynep Çelik Orhan +3

Pulsating detached eclipsing binary systems are crucial for studying the internal structure of oscillating stars. These systems are advantageous because binary effects on pulsation…

astro-ph.SR2025★ 4 cited

First detection of acoustic-like flux in the middle solar corona

V. Andretta, L. Abbo, G. Jerse +28

Waves are thought to play a significant role in the heating of the solar atmosphere and the acceleration of the wind. Among the many types of waves observed in the Sun, the so-call…

astro-ph.SR2025★ 2 cited

Discovery of the binary nature of the magnetospheric B-type star Oph A

M. E. Shultz, I. Berry, D. Bohlender +11

The nearby B-type star Oph A was recently identified as a rapidly rotating magnetic B-type star with variable radio and X-ray emission consistent with a magnetospheric origin.…

astro-ph.SR2024★ 1 cited

Super-slowly rotating Ap (ssrAp) stars: Spectroscopic study

G. Mathys, D. L. Holdsworth, M. Giarrusso +3

To gain better understanding of the Ap stars with the longest rotation periods, we obtained high resolution spectra of a sample of super-slowly rotating Ap (ssrAp) star candidates…

astro-ph.HE2024★ 7 cited

Galactic transient sources with the Cherenkov Telescope Array Observatory

Cherenkov Telescope Array Observatory Consortium

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exh…