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20072026
most citedMolecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments

762 citations · 5.1k across the 111 of their papers we have counts for

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9 papers · 1 filter

astro-ph.IM2022★ 17 cited

The Near Infrared Imager and Slitless Spectrograph for JWST -- V. Kernel Phase Imaging and Data Analysis

Jens Kammerer, Rachel A. Cooper, Thomas Vandal +26

Kernel phase imaging (KPI) enables the direct detection of substellar companions and circumstellar dust close to and below the classical (Rayleigh) diffraction limit. We present a…

astro-ph.IM2018

Planet Formation Imager: Project Update

John D. Monnier, Michael J. Ireland, Stefan Kraus +2

The Planet Formation Imager (PFI) is a near- and mid-infrared interferometer project with the driving science goal of imaging directly the key stages of planet formation, including…

astro-ph.IM2018

Hi-5: a potential high-contrast thermal near-infrared imager for the VLTI

D. Defrère, M. Ireland, O. Absil +25

Hi-5 is a high-contrast (or high dynamic range) infrared imager project for the VLTI. Its main goal is to characterize young extra-solar planetary systems and exozodiacal dust arou…

astro-ph.IM2018★ 55 cited

The path towards high-contrast imaging with the VLTI: the Hi-5 project

D. Defrère, O. Absil, J. -P. Berger +26

The development of high-contrast capabilities has long been recognized as one of the top priorities for the VLTI. As of today, the VLTI routinely achieves contrasts of a few 10$^{-…

astro-ph.IM2016★ 3 cited

Planet Formation Imager (PFI): science vision and key requirements

Stefan Kraus, John D. Monnier, Michael J. Ireland +75

The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes…

astro-ph.IM2016★ 56 cited

Observational calibration of the projection factor of Cepheids. II. Application to nine Cepheids with HST/FGS parallax measurements

Joanne Breitfelder, Antoine Mérand, Pierre Kervella +4

The distance to pulsating stars is classically estimated using the parallax-of-pulsation (PoP) method, which combines spectroscopic radial velocity measurements and angular diamete…