From January until April 2008 the MAGIC Telescope has been monitoring the radio galaxy M87 during several nights. A significant and variable signal has been...
MAAT: an IFU for GTC optimized using spectrograph wavefront measurements and superoptimization
The Mirror-slicer Array for Astronomical Transients (MAAT) is an IFU now being manufactured for the OSIRIS spectrograph on the 10.4-m GRANTECAN (GTC) telescope...
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...