iaa.es
Pablo studied a dual degree in Physics and Mathematics at the Complutense University of Madrid (UCM) and completed a Master’s in Theoretical Physics at the Autonomous University of Madrid (UAM), Spain. He joined the Institute of Astrophysics of Andalusia in June 2024 as a senior technician under the supervision of Dr. José Francisco Gómez to develop a source-search algorithm for the GASKAP-OH collaboration, a survey conducted with the ASKAP telescope (Australia Square Kilometre Array Pathfinder).
Pablo studied a dual degree in Physics and Mathematics at the Complutense University of Madrid (UCM) and completed a Master’s in Theoretical Physics at the Autonomous University of Madrid (UAM), Spain. He joined the Institute of Astrophysics of Andalusia in June 2024 as a senior technician under the supervision of Dr. José Francisco Gómez to develop a source-search algorithm for the GASKAP-OH collaboration, a survey conducted with the ASKAP telescope (Australia Square Kilometre Array Pathfinder).
Pablo studied a dual degree in Physics and Mathematics at the Complutense University of Madrid (UCM) and completed a Master’s in Theoretical Physics at the Autonomous University of Madrid (UAM). He is currently working as a senior technician under the supervision of Dr. José Francisco Gómez, focusing on the early and late stages of stellar evolution in the Milky Way and the Large Magellanic Cloud as part of the GASKAP-OH collaboration, a survey conducted with the ASKAP telescope (Australia Square Kilometre Array Pathfinder). His work primarily involves detecting sources from the data provided by the GASKAP-OH survey. Additionally, he studies masers in objects known as “Water Fountains,” which are associated with stars in the final stages of their evolution.
Pablo studied a dual degree in Physics and Mathematics at the Complutense University of Madrid (UCM) and completed a Master’s in Theoretical Physics at the Autonomous University of Madrid (UAM). He is currently working as a senior technician under the supervision of Dr. José Francisco Gómez, focusing on the early and late stages of stellar evolution in the Milky Way and the Large Magellanic Cloud as part of the GASKAP-OH collaboration, a survey conducted with the ASKAP telescope (Australia Square Kilometre Array Pathfinder). His work primarily involves detecting sources from the data provided by the GASKAP-OH survey. Additionally, he studies masers in objects known as “Water Fountains,” which are associated with stars in the final stages of their evolution.
