activity
20012024
most citedThe Gemini NICI Planet-Finding Campaign: The Frequency of Planets around Young Moving Group Stars

209 citations · 1.7k across the 32 of their papers we have counts for

collaborators

34 papers

astro-ph.IM2024

HARMONI at ELT: tolerance analysis and expected as-build imaging performance of the infrared spectrograph

Eduard Muslimov, Edgar Castillo-Dominguez, James Kariuki +6

HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470nm to 2450nm with resolving powers from 3300 to 180…

astro-ph.EP2024★ 22 cited

Behind the Mask: can HARMONI@ELT detect biosignatures in the reflected light of Proxima b?

Sophia R. Vaughan, Jayne L. Birkby, Niranjan Thatte +7

Proxima b is a rocky exoplanet in the habitable zone of the nearest star system and a key test case in the search for extraterrestrial life. Here, we investigate the characterizati…

astro-ph.IM2022

HARMONI at ELT: designing a laser guide star wavefront sensors for the ELT

Anne Costille, Anne Bonnefoi, Edgard Renault +16

HARMONI is the first light visible and near-IR integral field spectrograph for the ELT covering a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000…

astro-ph.IM2021★ 18 cited

HARMONI: the ELT's First-Light Near-infrared and Visible Integral Field Spectrograph

Niranjan Thatte, Matthias Tecza, Hermine Schnetler +13

The High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) is the visible and near-infrared (NIR), adaptive-optics-assisted, integral fi…

astro-ph.IM2020

Design of the HARMONI Pyramid WFS module

Noah Schwartz, Jean-François Sauvage, Edgard Renault +12

Current designs for all three extremely large telescopes show the overwhelming adoption of the pyramid wavefront sensor (P-WFS) as the WFS of choice for adaptive optics (AO) system…

astro-ph.IM2018★ 16 cited

Sensing and control of segmented mirrors with a pyramid wavefront sensor in the presence of spiders

Noah Schwartz, Jean-François Sauvage, Carlos Correia +9

The segmentation of the telescope pupil (by spiders & the segmented M4) create areas of phase isolated by the width of the spiders on the wavefront sensor (WFS), breaking the spati…