activity
20152018
most citedLaboratory and telescope demonstration of the TP3-WFS for the adaptive optics segment of AOLI

13 citations · 30 across the 5 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2018

The TP3-WFS: a new guy in town

Carlos Colodro-Conde, Sergio Velasco, Roberto López +11

The TP3-WFS (Two Pupil Plane Positions Wavefront Sensor) is, to the best of the authors' knowledge, the first physical implementation of the geometrical wavefront reconstruction al…

astro-ph.IM2018

Processing diffraction-limited images through innovative Super-Resolution techniques

E. Quevedo, S. Velasco, C. Colodro-Conde +10

In the ELTs era, where the need for versatile and innovative solutions to produce very high spatial resolution images has become a major issue, the search of synergies with other s…

astro-ph.IM2018

The adaptive optics lucky imager (AOLI): presentation, commissioning, and AIV innovations

Sergio Velasco, Carlos Colodro-Conde, Roberto L. López +6

Here we present the Adaptive Optics Lucky Imager (AOLI), a state-of-the-art instrument which makes use of two well proved techniques, Lucky Imaging (LI) and Adaptive Optics (AO), t…

astro-ph.IM2018

ALIOLI: Adaptive and Lucky Imaging Optics Lightweight Instrument

Sergio Velasco, Roberto L. López, Alejandro Oscoz +1

As a consequence of the evolution in the design and of the modularity of its components, AOLI for the William Herschel Telescope (WHT 4.2m) is much smaller and more efficient than…

astro-ph.IM20173 cited

P-REx: The Piston Reconstruction Experiment for Infrared Interferometry

Felix Widmann, Jörg-Uwe Pott, Sergio Velasco

For sensitive infrared interferometry, it is crucial to control the differential piston evolution between the used telescopes. This is classically done by the use of a fringe track…

astro-ph.GA20178 cited

Using binary statistics in Taurus-Auriga to distinguish between brown dwarf formation processes

M. Marks, E. L. Martín, V. J. S. Béjar +6

Whether BDs form as stars through gravitational collapse ("star-like") or BDs and some very low-mass stars constitute a separate population which form alongside stars comparable to…