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The wind-driven halo in high-contrast images I: analysis from the focal plane images of SPHERE
- Source :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, In press, Astronomy and Astrophysics-A&A, 2020, ⟨10.1051/0004-6361/201937397⟩, Astronomy & Astrophysics, 638, A98
- Publication Year :
- 2020
- Publisher :
- HAL CCSD, 2020.
-
Abstract
- Context. The wind driven halo is a feature observed within the images delivered by the latest generation of ground-based instruments equipped with an extreme adaptive optics system and a coronagraphic device, such as SPHERE at the VLT. This signature appears when the atmospheric turbulence conditions are varying faster than the adaptive optics loop can correct. The wind driven halo shows as a radial extension of the point spread function along a distinct direction (sometimes referred to as the butterfly pattern). When present, it significantly limits the contrast capabilities of the instrument and prevents the extraction of signals at close separation or extended signals such as circumstellar disks. This limitation is consequential because it contaminates the data a substantial fraction of the time: about 30% of the data produced by the VLT/SPHERE instrument are affected by the wind driven halo.Aims. This paper reviews the causes of the wind driven halo and presents a method to analyze its contribution directly from the scientific images. Its effect on the raw contrast and on the final contrast after post-processing is demonstrated.Methods. We used simulations and on-sky SPHERE data to verify that the parameters extracted with our method are capable of describing the wind driven halo present in the images. We studied the temporal, spatial and spectral variation of these parameters to point out its deleterious effect on the final contrast.Results. The data driven analysis we propose does provide information to accurately describe the wind driven halo contribution in the images. This analysis justifies why this is a fundamental limitation to the final contrast performance reached.Conclusions. With the established procedure, we will analyze a large sample of data delivered by SPHERE in order to propose, in the future, post-processing techniques tailored to remove the wind driven halo.<br />Astronomy and Astrophysics - A&A, EDP Sciences, In press
- Subjects :
- Point spread function
[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
media_common.quotation_subject
FOS: Physical sciences
Techniques: image processing
Context (language use)
Astrophysics
01 natural sciences
010309 optics
Infrared: planetary systems
0103 physical sciences
Contrast (vision)
Point (geometry)
Adaptive optics
010303 astronomy & astrophysics
Instrumentation and Methods for Astrophysics (astro-ph.IM)
media_common
Physics
Instrumentation: adaptive optics
Astronomy and Astrophysics
Atmospheric effects
Computational physics
Cardinal point
Space and Planetary Science
Feature (computer vision)
Instrumentation: high angular resolution
Halo
Astrophysics - Instrumentation and Methods for Astrophysics
Planet-disk interactions
Subjects
Details
- Language :
- English
- ISSN :
- 00046361
- Database :
- OpenAIRE
- Journal :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, In press, Astronomy and Astrophysics-A&A, 2020, ⟨10.1051/0004-6361/201937397⟩, Astronomy & Astrophysics, 638, A98
- Accession number :
- edsair.doi.dedup.....f0468c05ba364042e768fa5d49a6d758
- Full Text :
- https://doi.org/10.1051/0004-6361/201937397⟩