output
20082025
most citedDesign, analysis and test of a microdots apodizer for the Apodized Pupil Lyot Coronagraph

84 citations

6 papers

astro-ph.IM2025★ 1 cited

The New Science of Unidentified Aerospace-Undersea Phenomena (UAP)

Kevin H. Knuth, Philippe Ailleris, Hussein Ali Agrama +36

After decades of dismissal and secrecy, it has become clear that a significant number of the world's governments take Unidentified Aerospace-Undersea Phenomena (UAP), formerly know…

astro-ph.GA2022★ 56 cited

CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping

M. Bethermin, A. Gkogkou, M. Van Cuyck +27

The intensity mapping of the [CII] 158um line redshifted to the sub-mm window is a promising probe of the z>4 star formation and its spatial distribution into the large-scale struc…

astro-ph.IM2021★ 14 cited

CONCERTO at APEX: Installation and first phase of on-sky commissioning

A. Catalano, P. Ade, M. Aravena +40

CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn) is a large field-of-view (FoV) spectro-imager that has been installed on the Cassegrain Cabin of Atacama Pathfinder…

astro-ph2008★ 84 cited

Design, analysis and test of a microdots apodizer for the Apodized Pupil Lyot Coronagraph

P. Martinez, C. Dorrer, E. Aller Carpentier +4

Coronagraphic techniques are required to detect exoplanets with future Extremely Large Telescopes. One concept, the Apodized Pupil Lyot Coronagraph (APLC), is combining an apodizer…

astro-ph2008★ 23 cited

Comparison of coronagraphs for high contrast imaging in the context of Extremely Large Telescopes

P. Martinez, A. Boccaletti, M. Kasper +4

We compare coronagraph concepts and investigate their behavior and suitability for planet finder projects with Extremely Large Telescopes (ELTs, 30-42 meters class telescopes). For…

astro-ph2008★ 78 cited

Wavefront error correction and Earth-like planet detection by Self-Coherent Camera in space

R. Galicher, P. Baudoz, G. Rousset

In the context of exoplanet detection, the performance of coronagraphs is limited by wavefront errors. To efficiently correct for these aberrations with a deformable mirror, it is…