activity
20202023
most citedThe HOSTS survey for exozodiacal dust: Observational results from the complete survey

124 citations · 139 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2023

SHIMM as an atmospheric profiler on the Nickel Telescope

Ollie Jackson, Maaike A. M. van Kooten, Saavidra Perera +2

Optimal atmospheric conditions are beneficial for detecting exoplanets via high contrast imaging (HCI), as speckles from adaptive optics' (AO's) residuals can make it difficult to…

astro-ph.IM2023

GPI 2.0: Performance Evaluation of the Wavefront Sensor's EMCCD

Clarissa R. Do Ó, Saavidra Perera, Jérôme Maire +26

The Gemini Planet Imager (GPI) is a high contrast imaging instrument that aims to detect and characterize extrasolar planets. GPI is being upgraded to GPI 2.0, with several subsyst…

astro-ph.IM2023★ 14 cited

SHIMM: A Versatile Seeing Monitor for Astronomy

Saavidra Perera, Richard W. Wilson, Tim Butterley +3

Characterisation of atmospheric optical turbulence is crucial for the design and operation of modern ground-based optical telescopes. In particular, the effective application of ad…

astro-ph.IM2022★ 1 cited

Estimating effective wind speed from Gemini Planet Imager's adaptive optics data using covariance maps

Daniel M. Levinstein, Saavidra Perera, Quinn M. Konopacky +4

The Earth's turbulent atmosphere results in speckled and blurred images of astronomical objects when observed by ground based visible and near-infrared telescopes. Adaptive optics…

astro-ph.IM2021

P-REx II. Off-line Performance on VLTI/GRAVITY

Saavidra Perera, Jörg-Uwe Pott, Julien Woillez +4

For sensitive optical interferometry, it is crucial to control the evolution of the optical path difference (OPD) of the wavefront between the individual telescopes of the array. T…

astro-ph.SR2020★ 124 cited

The HOSTS survey for exozodiacal dust: Observational results from the complete survey

Steve Ertel, Denis Defrère, Philip M. Hinz +43

The Large Binocular Telescope Interferometer (LBTI) enables nulling interferometric observations across the N band (8 to 13 um) to suppress a star's bright light and probe for fain…