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SUMMARY:Marco Tarantino (University of Palermo)
DTSTART:20250326T121500Z
DTEND:20250326T130000Z
DTSTAMP:20260422T155330Z
UID:gbgstats/88
DESCRIPTION:Title: <a href="https://researchseminars.org/talk/gbgstats/88/
 ">Using a Neural Network approach and Starspots dependent models to predic
 t Effective Temperatures and Ages of young stars</a>\nby Marco Tarantino (
 University of Palermo) as part of Gothenburg statistics seminar\n\nLecture
  held in MVL14.\n\nAbstract\nThis study presents a statistical approach to
  accurately predict the effective temperatures of pre-main sequence stars\
 , which are necessary for determining stellar ages using the isochrone met
 hodology and cutting-age starspots-dependent models. By training a Neural 
 Network model on high-quality spectroscopic temperatures from the Gaia-ESO
  Survey as the response variable\, and using photometric data from Gaia DR
 3 and 2MASS catalogs as explanatory variables\, we implemented a methodolo
 gy to accurately derive the effective temperatures of much larger populati
 ons of stars for which only photometric data are available. The model demo
 nstrated robust performance for low-mass stars with temperatures below 700
 0 K\, including  young stars\, the primary focus of this work. Predicted t
 emperatures were employed to construct Hertzsprung-Russell diagrams and to
  predict stellar ages of different young clusters and star forming regions
  through isochrone interpolation\, achieving excellent agreement with spec
 troscopic-based ages and literature values derived from model-independent 
 methods like lithium equivalent widths. The inclusion of starspot evolutio
 nary models improved the age predictions\, providing a more accurate descr
 iption of stellar properties. Additionally\, the results regarding the eff
 ective temperature and age predictions of the young clusters provide evide
 nces of the presence of intrinsic age spreads in the youngest clusters\, s
 uggesting multiple formation events over time.\n
LOCATION:https://researchseminars.org/talk/gbgstats/88/
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