Hubble's Wide Field Camera 3 (WFC3) is the workhorse instrument for HST, providing direct (staring) and scanning modes using filters and grisms, covering from...
Machine Learning for Future Hyperspectral Data Analysis with the Hyperscout-H instrument on the ESA's Hera Mission
Introduction Hera is ESA's first planetary defense mission designed to characterize the binary near-Earth asteroid (65803) Didymos [1]. Its secondary component...
Macroturbulent broadening and its consequences on the study of rotational velocities and pulsations in massive stars
The analysis of high-resolution spectra of blue massive stars has allowed us to firmly ascertain the presence of an important non-rotational broadening in O and...
Macroturbulent broadening in Massive Stars and its possible connection to Stellar Oscillations
In this contribution, I review what we have learnt about macroturbulent broadening in the last decade and present first results of a long term observational...
MAD@VLT: Deep into the Madding Crowd of Omega Centauri
We present deep and accurate Near-Infrared (NIR) photometry of the Galactic Globular Cluster (GC) ω Cen. Data were collected using the Multi-Conjugate Adaptive...
Mag Waves in Sunspot Umbra: Slow Mode Leaking to the Corona
The linear oscillations of a stratified atmosphere embedded by a uniform vertical magnetic field are studied here. We use a simple theoretical model formed by...
Magellanic Cloud Emission Line Survey, Spectroscopy analisis
This work presents a low resolution spectroscopic data analisis of HII regions in the magellanic clouds. Nineteen nights of data over five observing seasons...
Magellanic Cloud Planetary Nebulae: probing the effects of metallicity on dust formation, mass-loss, and evolution.
Planetary nebulae (PNe) in the Magellanic Clouds (LMC, SMC) offer a unique opportunity to study both the population and evolution of low- and intermediate-mass...