An algorithm developed by researcher Andrés del Pino now applies Bayesian neural networks to data from the J-PLUS project. The aim is to robustly classify the astronomical objects detected by the survey and thus differentiate stars, quasars and galaxies. The research has been published in Astronomy and Astrophysics.
An article, led by CEFCA researcher Carlos López San Juan, focuses on those that are used for exoplanetary geology: white dwarfs with metals from the accretion of material from their planetary system. The research raises the contribution of the J-PLUS survey, developed from the Observatorio Astrofísico de Javalambre (OAJ), which now allows us to determine how the detection of these stars varies as they cool. The work has been published in Astronomy and Astrophysics.
Last February, the factory integration phase of the JAST80 telescope of the Observatorio Astrofísico de Javalambre (CEFCA) was completed. The telescope is assembled at Bamberg (Germany) where it is currently being tested with dummy optics. Preliminary tests show that the telescope can move with a velocity of up to 40 degrees per second, which makes T80 one of the worldwide fastest telescopes.
The brazilian partners of the Javalambre Physics of the Accelerated Universe Astrophysical Survey (J-PAS) collaboration, will put an identical replica of the OAJ JAST80 telescope of the Observatorio Astrofísico de Javalambre (CEFCA's observatory) in the Cerro Tololo Inter-American Observatory (CTIO), in Chile.
