We present a new method, the coupled escape probability (CEP), for exact calculation of line emission from multi-level systems, solving only algebraic equations...
A New Method Based on Artificial Neural Network Techniques for Determining the Fraction of Binaries in Star Clusters
We present a new method based on artificial neural networks techniques aimed at determining the fraction of binary systems populating star clusters. We address...
A new method for instrumental profile reconstruction of high-resolution spectrographs
GJ 9827 is a bright, nearby K7V star orbited by two super-Earths and one mini-Neptune on close-in orbits. The system was first discovered using K2 data and then...
A new method of measuring centre-of-mass velocities of radially pulsating stars from high-resolution spectroscopy
We present a radial velocity analysis of 20 solar neighbourhood RR Lyrae and three Population II Cepheid variables. We obtained high-resolution, moderate-to...
A new method of reconstructing images of gamma-ray telescopes applied to the LST-1 of CTAO
Context. Imaging atmospheric Cherenkov telescopes (IACTs) are used to observe very high-energy photons from the ground. Gamma rays are indirectly detected...
A new non-convex model of the binary asteroid (809) Lundia obtained with the SAGE modelling technique
We present a new non-convex model of the binary asteroid (809) Lundia. A SAGE (Shaping Asteroids with Genetic Evolution) method using disc-integrated photometry...
A new procedure for defining a homogenous line-list for solar-type stars
Context. The homogenization of the stellar parameters is an important goal for large observational spectroscopic surveys, but it is very difficult to achieve it...
We present a new puzzle involving Galactic microwave emission and attempt to resolve it. On one hand, a cross-correlation analysis of the Wisconsin Hα Mapper...
Helioseismic inversion techniques have been revealed as powerful tools for inferring the internal structure and dynamics of the Sun. One of the most popular...