We present a numerical code that solves the forward and inverse problem of the polarized radiative transfer equation in geometrical scale under the Zeeman regime. The code is fully parallelized, making it able to easily handle large observational and simulated datasets. We checked the reliability of the forward and inverse modules through different

The OSIRIS-REx asteroid sample-return mission is currently orbiting primitive near-Earth asteroid (101955) Bennu. Thousands of images are being acquired by the MapCam instrument onboard the spacecraft. In this work, we present preliminary results of a spectral clustering analysis applied to these color images.

The endohedral fullerene [Li@C60]+PF6− was characterized by differential scanning calorimetry (DSC), by electronic absorption spectroscopy in the spectral range from 195 to 800 nm and by FT-IR and far-infrared spectroscopy. [Li@C60]+PF6− shows a sharp melting point with the onset at 86 °C and peak at 90 °C and melting enthalpy of 9.5 kJ/mol. The

The distribution of galaxies on a colour-magnitude diagram reveals a bimodality, featuring a passively evolving red sequence and a star-forming blue cloud. The region between these two, the green valley (GV), represents a fundamental transition where quenching processes operate. We exploit an alternative definition of the GV using the 4000 Å break

Accurate line lists are crucial for correctly modelling a variety of astrophysical phenomena, including stellar photospheres and the atmospheres of extrasolar planets. This paper presents a new line database TOTO for the main isotopologues of titanium oxide (TiO): ^{46}Ti^{16}O, ^{47}Ti^{16}O, ^{48}Ti^{16}O, ^{49}Ti^{16}O, and ^{50}Ti^{16}O. The ^

The "European CMB Coordinator" group has a roadmap consisting of three axes: One is to build and deploy a 5m reflecting telescope at the South Pole; a second is to build and deploy 0.5m refracting telescopes in the Atacama Desert in Chile; and a third is to deploy low-frequency telescopes aimed at characterizing the sky in the 5-40 GHz range.