Detailed cool star flare morphology with CHEOPS and TESS***
Context. White-light stellar flares are proxies for some of the most energetic types of flares, but their triggering mechanism is still poorly understood. As...
Detailed Theoretical Predictions for the Outskirts of Dark Matter Halos
In the present work we describe the formalism necessary to derive the properties of dark matter halos beyond 2 virial radii using the spherical collapse model...
Detecting microvariability in type 2 quasars using enhanced F-test
Microvariability (intranight variability) is a low amplitude flux change at short time-scales (i.e. hours). It has been detected in unobscured type 1 active...
Detecting outliers in astronomical images with deep generative networks
With the advent of future big-data surveys, automated tools for unsupervised discovery are becoming ever more necessary. In this work, we explore the ability of...
Detecting planets around very cool dwarfs at near infrared wavelengths with the radial velocity technique
Context. Radial velocity monitoring of very cool dwarfs such as late M- and hot L-dwarfs has become a promising tool in the search for rocky planets as well as...
Detection and temporal coherence of p-modes below 1.4 mHz
Data collected recently by the helioseismic experiments aboard the SOHO spacecraft have allowed the detection of low degree p-modes with increasingly lower...
As a parallel result of an IT Project aimed at determining accurate distances to more than 30 planetary nebulae using the extinction-distance method, we report...
Detection of a high-velocity sodium feature on the ultra-hot Jupiter WASP-121 b
Context. Ultra-hot Jupiters, with their high equilibrium temperatures and resolved spectral lines, have emerged as a perfect testbed for new analysis techniques...