Coherent differential imaging of high-contrast extended sources with VLT/SPHERE
Context. High-contrast imaging relies on advanced coronagraphs and adaptive optics (AO) to attenuate the starlight. However, residual aberrations, especially non-common path aberrations between the AO channel and the coronagraph channel, limit the instrument performance. While post-processing techniques such as spectral or angular differential imaging (ADI) can partially address those issues, they suffer from self-subtraction and inefficiencies at small angular separations or when observations are conducted far from transit. Aims. We previously demonstrated the on-sky performance of coherent differential imaging (CDI), which offers a promising alternative. It allows for isolating coherent starlight residuals through speckle modulation, which can then be subtracted from the raw images during post-processing. This work aims to validate a CDI method on real science targets using VLT/SPHERE, demonstrating its effectiveness in imaging almost face-on circumstellar disks, which are typically challenging to retrieve with ADI. Methods. We temporally modulated the speckle field in VLT/SPHERE images, applying small phase offsets on the AO deformable mirror while observing stars surrounded by circumstellar material: HR 4796A, CPD-36 6759, HD 169142, and HD 163296. We hence separated the astrophysical scene from the stellar speckle field, whose lights are mutually incoherent. Results. Combining a dozen of data frames and reference coronagraph point spread functions through a Karhunen–Loève image projection framework, we recover the circumstellar disks without the artifacts that are usually introduced by common post-processing algorithms (e.g., self-subtraction). Conclusions. The CDI method therefore represents a promising strategy for calibrating the effect of static and quasi-static aberrations in future direct imaging surveys. Indeed, it is efficient, does not require frequent telescope slewing, and does not introduce image artifacts to first order.
Authors
- Z. Wahhaj (ORCID: https://orcid.org/0000-0001-8269-324X)
- Pierre Baudoz (ORCID: https://orcid.org/0000-0002-2711-7116)
- G. Chauvin (ORCID: https://orcid.org/0000-0003-4022-8598)
- Axel Potier (ORCID: https://orcid.org/0000-0002-1153-3385)
- Johan Mazoyer
- Jonas Kühn (ORCID: https://orcid.org/0000-0002-6344-4835)
- Raphaël Galicher
- Ruben Tandon
- Laura Perez
Publication Details
- Journal
- Springer Link (Chiba Institute of Technology)
- Published
- 2025-12-08
- DOI
- https://doi.org/10.1051/0004-6361/202556606/pdf
- Primary Topic
- Stellar, planetary, and galactic studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00