ConferencePaper
Proceedings of the International Astronomical Union  (2025)

Bayesian deconvolution of a rotating spectral line profile to a non-rotating one

Curé; M.; Escárate; P.; Celedón; L.; Cavieres; J.; Olivares; E.; Araya; I.; Arcos; C.; Pezoa; R.; Farías; G.; Machuca; N.

Keywords: methods: numerical; methods: statistical; stars: rotation; techniques: spectroscopic

Abstract

In this work we present a Bayesian approach to obtain the non-rotating stellar spectra from an observed spectrum of a rotating star. This is our first attempt to solve an inverse problem expressed in terms of a Fredholm integral. Our preliminary results with synthetic spectra are promising. More studies are required to compare our Bayesian approach with the standard method for real spectra. © The Author(s), 2025. Published by Cambridge University Press on behalf of International Astronomical Union.

Más información

Título de la Revista: Proceedings of the International Astronomical Union
Volumen: 19
Número: S368
Editorial: Cambridge University Press
Fecha de publicación: 2025
Página de inicio: 107
Página final: 109
Idioma: English
DOI:

10.1017/S1743921322003532