activity
20032020
most citedStrong atom-field coupling for Bose-Einstein condensates in an optical cavity on a chip

701 citations · 2.8k across the 21 of their papers we have counts for

collaborators

22 papers

astro-ph.IM2020★ 19 cited

Measuring and characterizing the line profile of HARPS with a laser frequency comb

Fei Zhao, G. Lo Curto, L. Pasquini +13

Aims. We study the 2D spectral line profile of HARPS (High Accuracy Radial Velocity Planet Searcher), measuring its variation with position across the detector and with changing li…

astro-ph.SR2020★ 37 cited

The solar gravitational redshift from HARPS-LFC Moon spectra. A test of the General Theory of Relativity

J. I. González Hernández, R. Rebolo, L. Pasquini +15

The General Theory of Relativity predicts the redshift of spectral lines in the solar photosphere, as a consequence of the gravitational potential of the Sun. This effect can be me…

astro-ph.IM2020★ 172 cited

SPIRou: nIR velocimetry & spectropolarimetry at the CFHT

J. -F. Donati, D. Kouach, C. Moutou +63

This paper presents an overview of SPIRou, the new-generation near-infrared spectropolarimeter / precision velocimeter recently installed on the 3.6-m Canada-France-Hawaii Telescop…

astro-ph.IM2020★ 76 cited

Performance Verification of the EXtreme PREcision Spectrograph

Ryan T. Blackman, Debra A. Fischer, Colby A. Jurgenson +25

The EXtreme PREcision Spectrograph (EXPRES) is a new Doppler spectrograph designed to reach a radial velocity measurement precision sufficient to detect Earth-like exoplanets orbit…

astro-ph.IM2020★ 57 cited

A crucial test for astronomical spectrograph calibration with frequency combs

Rafael A. Probst, Dinko Milaković, Borja Toledo-Padrón +23

Laser frequency combs (LFCs) are well on their way to becoming the next-generation calibration sources for precision astronomical spectroscopy. This development is considered key i…

astro-ph.SR2019★ 55 cited

Convective blueshifts in the solar atmosphere: III. High-accuracy observations of spectral lines in the visible

Johannes Löhner-Böttcher, Wolfgang Schmidt, Rolf Schlichenmaier +2

Convective motions in the solar atmosphere cause spectral lines to become asymmetric and shifted in wavelength. For photospheric lines, this differential Doppler shift varies from…