Determining Stellar Elemental Abundances from DESI Spectra with the Data-driven Payne
Stellar abundances for a large number of stars provide key information for the study of Galactic formation history. Large spectroscopic surveys such as the Dark Energy Spectroscopic Instrument (DESI) and LAMOST take median-to-low-resolution ( R ≲ 5000) spectra in the full optical wavelength range fo...
I tiakina i:
| Ngā kaituhi matua: | , , , , , , , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2024-01-01
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| Rangatū: | The Astrophysical Journal Supplement Series |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/1538-4365/ad51dd |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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