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TZID:US/Arizona
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DTSTART:20221106T000000
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SUMMARY:Using Open Science Studio platform to study structural relationshi
 ps of remote galaxies from the CANDELS catalogs - Guillermo Valé Arteaga
 \, Ramon E. Ramirez-Linan
DTSTART;TZID=US/Arizona:20231106T083000
DTEND;TZID=US/Arizona:20231106T083000
DTSTAMP:20260915T030250Z
UID:pretalx-adass2023-FFLFQV@pretalx.com
DESCRIPTION:Using an Open Source Platform that Navteca is deploying for NA
 SA Astrophysics\, I was able to complete my degree final thesis at the Uni
 versidad complutense de Madrid\, this research is an example of why NASA's
  initiative to Open Science is so important and can have a global impact o
 n science students and researchers.\n\nThis project aims to be an explorat
 ory investigation of the structural relationships of remote galaxies at re
 dshift values ranging between 1.5 and 2.5 using the CANDELS and 3D-HST cat
 alogs. To do so\, data analysis tools with Python will be employed. Variou
 s physical properties of the galaxies will be studied\, such as stellar ma
 ss\, star formation rate and luminosity. In addition\, visualization and s
 tatistical analysis techniques will be used to identify the most important
  relationships between these properties and thus gain a better understandi
 ng of the formation and evolution of remote galaxies. Data analysis will a
 llow establishing relationships between the studied properties\, which wil
 l contribute to the understanding of the formation and evolution of galaxi
 es. \n\nFurthermore\, the use of machine learning techniques will be imple
 mented to predict a particular physical property as a function other param
 eters. We demonstrate the feasibility of this approach by training models 
 using a large dataset of galactic physical properties and validating the a
 ccuracy of the predicted property against experimental data. Our results c
 ould show that machine learning models might provide a promising avenue fo
 r predicting desired galactic properties with high accuracy and efficiency
 \, potentially enabling new insights and applications in extragalactic ast
 rophysics and beyond.
LOCATION:Posters
URL:https://pretalx.com/adass2023/talk/FFLFQV/
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