SD1000 Collaboration: Hunting down the subdwarf populations
Peter Nemeth, Roy {\O}stensen, Joris Vos, Adela Kawka, Stephane Vennes

TL;DR
This paper presents updated methods for spectral analysis aimed at distinguishing subdwarf populations, providing insights into their formation and atmospheric diversity, within the context of the SD1000 collaboration.
Contribution
It introduces a new standardized spectral analysis method developed over a year for studying subdwarf populations in SD1000.
Findings
Enhanced spectral analysis techniques for subdwarfs
Standardized method adopted by SD1000
Insights into subdwarf formation and atmospheric processes
Abstract
Separating the subdwarf populations may shed light on their formation history and give unique insights into the atmospheric processes that are thought to be responsible for their abundance diversity. Such a task requires complex and time consuming spectral analyses, which we started to tailor to our objectives a year ago. Here we report the updates that have been made over the past year and will be the standard method in SD1000.
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Taxonomy
TopicsAtmospheric and Environmental Gas Dynamics · Atmospheric Ozone and Climate · Meteorological Phenomena and Simulations
