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Imaging exoplanets with coronagraphic instruments

open access: yesComptes Rendus. Physique, 2023
Exoplanetary science is a very active field of astronomy nowadays, with questions still opened such as how planetary systems form and evolve (occurrence, process), why such a diversity of exoplanets is observed (mass, radius, orbital parameters ...
Galicher, Raphaël, Mazoyer, Johan
doaj   +6 more sources

Speckle noise and dynamic range in coronagraphic images [PDF]

open access: yesThe Astrophysical Journal, 2007
This paper is concerned with the theoretical properties of high contrast coronagraphic images in the context of exoplanet searches. We derive and analyze the statistical properties of the residual starlight in coronagraphic images, and describe the ...
Andre Ferrari   +15 more
core   +4 more sources

MEMS Deformable Mirrors for Space-Based High-Contrast Imaging [PDF]

open access: yesMicromachines, 2019
Micro-Electro-Mechanical Systems (MEMS) Deformable Mirrors (DMs) enable precise wavefront control for optical systems. This technology can be used to meet the extreme wavefront control requirements for high contrast imaging of exoplanets with coronagraph
Rachel E. Morgan   +19 more
doaj   +2 more sources

High contrast imaging wavefront sensor referencing from coronagraphic images [PDF]

open access: yesTechniques and Instrumentation for Detection of Exoplanets X, 2021
A key challenge of high contrast imaging (HCI) is to differentiate a speckle from an exoplanet signal. The sources of speckles are a combination of atmospheric residuals and aberrations in the non-common path. Those non-common path aberrations (NCPA) are particularly challenging to compensate for as they are not directly measured, and because they ...
Skaf, Nour   +13 more
openaire   +2 more sources

Coronagraphic phase diversity: performance study and laboratory demonstration [PDF]

open access: yes, 2013
The final performance of current and future instruments dedicated to exoplanet detection and characterization (such as SPHERE on the European Very Large Telescope, GPI on Gemini North, or future instruments on Extremely Large Telescopes) is limited by ...
Mugnier, L. M.   +2 more
core   +16 more sources

Speckle lifetime in XAO coronagraphic images: temporal evolution of SPHERE coronagraphic images [PDF]

open access: yesSPIE Proceedings, 2016
18 pages, 20 ...
Milli, J.   +16 more
openaire   +3 more sources

Rectangular-Mask Coronagraphs for High-Contrast Imaging [PDF]

open access: yesThe Astrophysical Journal, 2004
We present yet another new family of masks for high-contrast imaging as required for the to-be-built terrestrial planet finder space telescope. The ``best'' design involves a square entrance pupil having a 4-vane spider, a square image-plane mask containing a plus-sign shaped occulter to block the starlight inside 0.6 lambda/D, and a Lyot-plane mask ...
Vanderbei, Robert J.   +2 more
openaire   +3 more sources

First Observations of the Brown Dwarf HD 19467 B with JWST

open access: yesThe Astrophysical Journal, 2023
We observed HD 19467 B with JWST’s NIRCam in six filters spanning 2.5–4.6 μ m with the long-wavelength bar coronagraph. The brown dwarf HD 19467 B was initially identified through a long-period trend in the radial velocity of the G3V star HD 19467.
Alexandra Z. Greenbaum   +23 more
doaj   +1 more source

Hiding Dust around ϵ Eridani

open access: yesThe Astronomical Journal, 2023
With a Jupiter-like exoplanet and a debris disk with both asteroid and Kuiper Belt analogs, ϵ Eridani has a fascinating resemblance to our expectations for a young solar system.
Schuyler Grace Wolff   +4 more
doaj   +1 more source

Square Root Compression and Noise Effects in Digitally Transformed Images

open access: yesThe Astrophysical Journal, 2022
We report on a particular example of noise and data representation interacting to introduce systematic error into scientific measurements. Many instruments collect integer digitized values and apply nonlinear coding, in particular square root coding, to ...
Craig E. DeForest   +3 more
doaj   +1 more source

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