activity
20102016
most citedOptical flux behaviour of a sample of Fermi blazars

15 citations · 23 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2016★ 15 cited

Optical flux behaviour of a sample of Fermi blazars

E. J. Marchesini, I. Andruchow, S. A. Cellone +7

Aims: We aim at investigating the time-behaviour of a sample of gamma-ray blazars. We present the results from a 13 month-long optical photometry monitoring campaign of the blazars…

astro-ph.HE2015★ 1 cited

Real-time evolution of a large-scale relativistic jet

Josep Martí, Pedro L. Luque-Escamilla, Gustavo E. Romero +2

Context. Astrophysical jets are ubiquitous in the Universe on all scales, but their large-scale dynamics and evolution in time are hard to observe since they usually develop at a v…

astro-ph.HE2013★ 7 cited

The star forming region Monoceros R2 as a gamma-ray source

Josep Martí, Pedro L. Luque-Escamilla, Álvaro J. Muñoz-Arjonilla +6

Context. After the release of the gamma-ray source catalog produced by the Fermi satellite during its first two years of operation, a significant fraction of sources still remain u…

astro-ph.HE2011

Infrared and radio study of the W43 cluster: resolved binaries and non-thermal emission

P. L. Luque-Escamilla, A. J. Muñoz-Arjonilla, J. R. Sánchez-Sutil +3

Context: The recent detection of very high-energy (VHE) gamma-ray emission from the direction of the W43 star-forming region prompted us to investigate its stellar population in de…

astro-ph.HE2011

Are T Tauri stars gamma-ray emitters?

María Victoria del Valle, Gustavo E. Romero, Pedro Luis Luque-Escamilla +2

T Tauri stars are young, low mass, pre-main sequence stars surrounded by an accretion disk. These objects present strong magnetic activity and powerful magnetic reconnection events…

astro-ph.HE2010

Identification of the optical and near-infrared counterpart of GRS 1758-258

A. J. Muñoz-Arjonilla, J. Martí, P. L. Luque-Escamilla +4

Context. Understood to be a microquasar in the Galactic center region, GRS 1758-258 has not yet been unambiguously identified to have an optical/near-infrared counterpart, mainly b…