G. Cugno

TL;DR: In recent years, our understanding of giant planet formation progressed substantially as mentioned in this paper, and there have even been detections of a few young protoplanet candidates still embedded in the circumste...

TL;DR: In this article, the authors detect and quantify observables related to accretion processes occurring locally in circumstellar disks, which could be attributed to young forming planets, focusing on objects known to host protoplanet candidates and/or disk structures that are the result of interactions with planets.

TL;DR: PynPoint as mentioned in this paper is a data-reduction pipeline for processing and analysis of high-contrast imaging data obtained with pupil-stabilized observations, which is particularly suitable for the 3-5 μm wavelength range where typically thousands of frames have to be processed and an accurate subtraction of the thermal background emission is critical.

TL;DR: In this paper, the authors used the angular spectral differential imaging (ASDI) and principal component analysis (PCA) to reduce the ZIMPOL pupil stabilized data by applying the method of ASDI, which combines both techniques.

TL;DR: In this article, the authors presented new L' and M' observations of the HIP 65426 b from the NACO instrument at the VLT from the SPHERE-SHINE survey.