activity
20102021
most citedSensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

135 citations · 419 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.HE2021★ 3 cited

Orbital and sub-orbital period determination of the candidate high-mass X-ray binary HD 3191

Josep Martí, Pedro L. Luque-Escamilla, Estrella Sánchez-Ayaso +1

The final aim of this paper is to expand the sparse group of X-ray binaries with gamma-ray counterparts as laboratories to study high-energy processes under physical conditions tha…

astro-ph.HE2020★ 3 cited

Effects of precession versus instabilities on the jets of GRS 1758-258

Pedro L. Luque-Escamilla, Josep Martí, José Martínez-Aroza

Aims. The prototypical microquasar GRS 1758-258 exhibits large-scale morphological changes in radio maps over time which have been attributed to the rise of instabilities. Here, we…

astro-ph.HE2020★ 77 cited

Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

The Cherenkov Telescope Array Consortium, :, H. Abdalla +496

The Cherenkov Telescope Array (CTA), the new-generation ground-based observatory for -ray astronomy, provides unique capabilities to address significant open questions in astrop…

astro-ph.HE2020★ 135 cited

Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

The Cherenkov Telescope Array Consortium, :, A. Acharyya +449

We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray sig…

astro-ph.HE2020★ 8 cited

A blazar as the likely counterpart to 4FGL J0647.7-4418 instead of a gamma-ray binary

Josep Martí, Estrella Sánchez-Ayaso, Pedro L. Luque-Escamilla +3

The persistent gamma-ray source 4FGL J0647.7-4418 is tentatively associated in the latest Fermi catalogue with the sub-dwarf O-type X-ray binary HD 49798. However, an AGN candidate…

astro-ph.SR2018★ 1 cited

Detection of optical flickering from the symbiotic Mira-type binary star EF Aquilae

V. V. Dimitrov, S. Boeva, J. Martí +8

We performed photometry with a 1 minute time resolution of the symbiotic stars EF Aquilae, AG Pegasi and SU Lyncis in Johnson B and V band. Our observations of the symbiotic Mira-t…