Published 2024 | Version v3

LAMA: LAMOST Medium Resolution Spectral Analysis Pipeline

Authors/Creators

  • 1. ROR icon National Astronomical Observatories

Description

LAMA is used to estimate the stellar parameters, including Teff, logg, [Fe/H], RV and vsini from LAMOST-MRS spectrum.

LAMA.py: the main code of LAMA

air2vac.py: a function to convert the wavelength from air to vaccum.

mod2fits.py: generates a fits file from the binary files of templates.

norm.py: normalizes the spectrum.

rv_xcor.py: calculates the Cross-Correlation Function between observed and template spectra.

 

The catalog of stellar parameters estimated by LAMA:

LAMA_stars_Readme.txt

LAMA_stars.csv

LAMA_stars.fits

LAMA_stars.dat

The catalog of spectral stellar parameters estimated by LAMA:

LAMA_spec_Readme.txt

LAMA_spec.csv

LAMA_spec.fits

LAMA_spec.dat

Files

LAMA_stars_Readme.txt

Files (4.2 GB)

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Additional details

Software