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[PDF] Top 20 Vortex Image Processing (VIP) package for high-contrast direct imaging

Has 10000 "Vortex Image Processing (VIP) package for high-contrast direct imaging" found on our website. Below are the top 20 most common "Vortex Image Processing (VIP) package for high-contrast direct imaging".

Vortex Image Processing (VIP) package for high-contrast direct imaging

Vortex Image Processing (VIP) package for high-contrast direct imaging

... framework for reproducible and robust data ...three high- contrast imaging observational techniques: angular, reference-star and multi- spectral differential ... Voir le document complet

1

VIP: Vortex Image Processing package for high-contrast direct imaging

VIP: Vortex Image Processing package for high-contrast direct imaging

... VIP for the case of ADI data, it includes several types of low-rank matrix approximations for reference PSF subtraction, such as the LLSG decomposition, and PCA- and NMF-based ...of processing big, ... Voir le document complet

12

Advanced data processing for high-contrast imaging - Pushing exoplanet direct detection limits with machine learning

Advanced data processing for high-contrast imaging - Pushing exoplanet direct detection limits with machine learning

... data processing in high- contrast ...Data processing constitutes a critical component of high-contrast imaging, as advanced image processing algorithms are ... Voir le document complet

203

CHIPS: The Carina High-contrast Imaging Project of massive Stars

CHIPS: The Carina High-contrast Imaging Project of massive Stars

... at High angular res- olutions survey (SMaSH+, Sana et ...other high contrast imaging campaigns (Turner et ...flux contrast of Δmag = 10 at separations as close as ...the Vortex ... Voir le document complet

1

A review of high contrast imaging modes for METIS

A review of high contrast imaging modes for METIS

... 2018). High-frequency chopping is not required to monitor the sky emission at these ...LM-band vortex coronagraphy, accurate sky subtraction is generally performed based on the science frames themselves, at ... Voir le document complet

12

Supervised detection of exoplanets in high-contrast imaging sequences

Supervised detection of exoplanets in high-contrast imaging sequences

... community for generating synthetic data and assessing the sensitivity lim- its of image-processing algorithms and ...planet-to-star contrast) is too low, in which case the signature of the ... Voir le document complet

13

Small-angle, high-contrast exoplanet imaging with the L-band AGPM vector vortex coronagraph now offered at the VLT

Small-angle, high-contrast exoplanet imaging with the L-band AGPM vector vortex coronagraph now offered at the VLT

... at 2λ/D), which is more than needed for on-sky operations where the limit is set by the residual wavefront aberrations. The AGPM was installed inside NACO as part of a planned overhaul in November 2012. The AGPM ... Voir le document complet

9

The Subaru Coronagraphic Extreme Adaptive Optics System: Enabling High-Contrast Imaging on Solar-System Scales

The Subaru Coronagraphic Extreme Adaptive Optics System: Enabling High-Contrast Imaging on Solar-System Scales

... multipurpose high- contrast imaging platform designed for the discovery and detailed characterization of exoplanetary systems and serves as a testbed for high-contrast ... Voir le document complet

20

Astrometric and photometric accuracies in high contrast imaging: The SPHERE speckle calibration tool (SpeCal)

Astrometric and photometric accuracies in high contrast imaging: The SPHERE speckle calibration tool (SpeCal)

... correcting for instrumental artifacts. This includes image pro- cessing steps such as flat-fielding, bad pixels, background, frame selection, anamorphism correction, true north alignment, frame centring, ... Voir le document complet

11

Astrometric and photometric accuracies in high contrast imaging: The SPHERE speckle calibration tool (SpeCal)⋆

Astrometric and photometric accuracies in high contrast imaging: The SPHERE speckle calibration tool (SpeCal)⋆

... correcting for instrumental artifacts. This includes image pro- cessing steps such as flat-fielding, bad pixels, background, frame selection, anamorphism correction, true north alignment, frame centring, ... Voir le document complet

12

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

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

... maturity for the the thermal near-infrared (L and M bands), a sweet spot to image young giant ...the contrast of long-baseline interferometers ...tracking, high-dispersion interferometry). ... Voir le document complet

24

An automated image-processing pipeline for high-throughput analysis of root architecture in OpenAlea

An automated image-processing pipeline for high-throughput analysis of root architecture in OpenAlea

... 3. Estimation of a root architecture The root architecture is obtained by converting the root graph to an axial tree structure (Godin et al., 1998). This is done in two passes. First the graph is converted to a tree ... Voir le document complet

4

High-contrast OLEDs with high-efficiency

High-contrast OLEDs with high-efficiency

... 1999). For that reason, metals with relatively large k are required for this type of coatings (see ...compensate for the increase of optical thickness in the dielectrics at shorter ...nk/λ for ... Voir le document complet

19

Direct matching for improving image-based registration

Direct matching for improving image-based registration

... vision, direct methods solve the problem by minimizing the photometric and the geometric error directly in sensor space as opposed to ICP (Iterative closest point) or feature-based image approaches which ... Voir le document complet

2

Computational Imaging for VLBI Image Reconstruction

Computational Imaging for VLBI Image Reconstruction

... For mm/sub-mm wavelength VLBI, reconstruction is complicated by corruption of the visibility phases. CLEAN is not inherently capable of handling this problem; however, self-calibration methods have been developed ... Voir le document complet

11

Dynamic contrast for overcoming spectral interferences in fluorescence imaging

Dynamic contrast for overcoming spectral interferences in fluorescence imaging

... Dynamic contrast for overcoming spectral interferences in fluorescence imaging 9 observation under constant ...enabling for full- frame ... Voir le document complet

15

Contrast enhancement of propagation based X-ray phase contrast imaging

Contrast enhancement of propagation based X-ray phase contrast imaging

... phase contrast imaging (XPCI) technique derived from propagation depen- dent phase ...CT imaging of a human artery specimen with extensive atherosclerotic ...phase contrast was greatly ... Voir le document complet

12

Anamorphic image processing

Anamorphic image processing

... The lines of projection are parallel and intersect the view plane at an oblique angle, thereby providing a view of object depth.. The face of the object that is parallel [r] ... Voir le document complet

56

A search for accreting young companions embedded in circumstellar disks. High-contrast Hα imaging with VLT/SPHERE

A search for accreting young companions embedded in circumstellar disks. High-contrast Hα imaging with VLT/SPHERE

... look for accretion signatures from gas falling onto the planet and its ...). High-contrast imaging using Hα filters was already successfully applied in three ...differential imaging ... Voir le document complet

20

Curve-and-Surface Evolutions for Image Processing

Curve-and-Surface Evolutions for Image Processing

... une image bruit´ ee par un bruit gaussien, c’est-` a-dire que g = g 0 + n o` u g 0 est l’image id´ eale (celle qu’on veut observer) et n est un bruit dont les oscillations sont suppos´ ees bien plus rapides que ... Voir le document complet

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