A low-cost chopping system and uncooled microbolometer array for ground-based astronomy
Mid-Infrared imaging is vital for the study of a wide variety of astronomical phenomena, including evolved stars, exoplanets, and dust enshrouded processes such...
A machine learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps with The Three Hundred clusters
Our study introduces a new machine learning algorithm for estimating 3D cumulative radial profiles of total and gas mass in galaxy clusters from thermal Sunyaev...
One of the most useful diagnostic tools for the detection of inclined magnetic fields in solar chromospheric and coronal structures is that based on the fact...
A major step in understanding the X-ray generation in comets: recent progress obtained with XMM-Newton
The observation of comet C/2000 WM1 (LINEAR) with XMM-Newton is a highlight in the field of cometary research. During 17 hours of almost uninterrupted...
A map-making algorithm for the QUIJOTE CMB experiment
In the last years we obtained a very detailed picture of the Primordial Universe by, among other means, measuring the intensity and the polarization of the...
A mask quality control tool for the OSIRIS multi-object spectrograph
OSIRIS multi object spectrograph uses a set of user-customised-masks, which are manufactured on-demand. The manufacturing process consists of drilling the...
A Massive AGB Star as Source of Short-Lived Nuclei in the Early Solar System
The origin of short-lived radioactive nuclei at the time of the formation of the Sun is a much debated mystery in modern astronomy. We show that abundance...