activity
20152022
most citedNear-Earth asteroids spectroscopic survey at Isaac Newton Telescope

36 citations · 92 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.IM20222 cited

Costs and benefits of automation for astronomical facilities

A. Yanes-Díaz, S. Rueda-Teruel, R. Bello +57

The Observatorio Astrofísico de Javalambre (OAJ†1) in Spain is a young astronomical facility, conceived and developed from the beginning as a fully automated observatory with the m…

astro-ph.GA2021

Study of the open cluster Alessi-Teutsch 9 (ASCC 10) using multiband photometry and Gaia EDR3

Nestor Sanchez, Fatima Lopez-Martinez, Sandra Ocando +1

There is a growing interest in the automated characterization of open clusters using data from the Gaia mission. This work evidences the importance of choosing an appropriate sampl…

astro-ph.GA20209 cited

A catalogue of open cluster radii determined from Gaia proper motions

Nestor Sanchez, Emilio Alfaro, Fatima Lopez-Martinez

In this work we improve a previously published method to calculate in a reliable way the radius of an open cluster. The method is based on the behaviour of stars in the proper moti…

astro-ph.EP201936 cited

Near-Earth asteroids spectroscopic survey at Isaac Newton Telescope

M. Popescu, O. Vaduvescu, J. de León +15

The population of near-Earth asteroids (NEAs) shows a large variety of objects in terms of physical and dynamical properties. They are subject to planetary encounters and to strong…

astro-ph.HE2018

The 1989 and 2015 outbursts of V404 Cygni: a global study of wind-related optical features

D. Mata Sánchez, T. Muñoz-Darias, J. Casares +19

The black hole transient V404 Cygni exhibited a bright outburst in June 2015 that was intensively followed over a wide range of wavelengths. Our team obtained high time resolution…

astro-ph.GA20189 cited

A method for determining the radius of an open cluster from stellar proper motions

Nestor Sanchez, Emilio J. Alfaro, Fatima Lopez-Martinez

We propose a method for calculating the radius of an open cluster in an objective way from an astrometric catalogue containing, at least, positions and proper motions. It uses the…