Table 1.

Typical accuracies of atmospheric parameters determined with LSP3 for stars of spectral signal-to-nose ratios > 20 and >50.

Teff [K]|$\log \, g$| [dex][Fe/H] [dex][α/Fe] [dex]Vr [|$\rm km\, s^{-1}$|]MV [mag]MKs [mag]
SNRs > 201500.20.150.150.5–0.60.5–0.6
SNRs > 501000.10.10.0550.2–0.30.2–0.3
Teff [K]|$\log \, g$| [dex][Fe/H] [dex][α/Fe] [dex]Vr [|$\rm km\, s^{-1}$|]MV [mag]MKs [mag]
SNRs > 201500.20.150.150.5–0.60.5–0.6
SNRs > 501000.10.10.0550.2–0.30.2–0.3
Table 1.

Typical accuracies of atmospheric parameters determined with LSP3 for stars of spectral signal-to-nose ratios > 20 and >50.

Teff [K]|$\log \, g$| [dex][Fe/H] [dex][α/Fe] [dex]Vr [|$\rm km\, s^{-1}$|]MV [mag]MKs [mag]
SNRs > 201500.20.150.150.5–0.60.5–0.6
SNRs > 501000.10.10.0550.2–0.30.2–0.3
Teff [K]|$\log \, g$| [dex][Fe/H] [dex][α/Fe] [dex]Vr [|$\rm km\, s^{-1}$|]MV [mag]MKs [mag]
SNRs > 201500.20.150.150.5–0.60.5–0.6
SNRs > 501000.10.10.0550.2–0.30.2–0.3
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close