MKCLASS: An expert stellar spectral classification system


MKCLASS is a program designed to classify stellar spectra on the MK system in a way similar to humans, via direct comparison with MK standards. The program is described in the following documents:

Documentation

Documentation - Installation and Use

Journal paper (preprint)

Before you attempt to use MKCLASS, you may first wish to download and install the program XCLASS, which is a manual spectral classification program which uses the same standard spectrum libraries as MKCLASS. See below for documentation and source code for XCLASS.

Download source code and spectral libraries


mkclassv107.tar.gz

mklib.tar.gz

Standards used in the spectral libraries


libnor36 standards


Version History

v1.07: Sept 10, 2015. General improvement of the quality of spectral types from B -- M, including improved recognition of carbon stars, Wolf Rayet stars, white dwarfs and other non-MK types. Improved classification of chemically peculiar stars. This is the version used to classify LAMOST spectra in the Kepler field (submitted).
v1.05: July 14, 2014. Upgraded quality evaluation of late-K and M-type stars.
v1.04: July 9, 2014. Improvements in the determination of the metallicity type of A and F-type stars.
v1.03: June 29, 2014. Introduced improvements in the identification of emission-line stars, and in the luminosity classification of mid A-type stars. Also introduced the use of an environment variable to take care of a non-standard location for the mklib standards libraries.
v1.02: Improved the classification of metal-weak A-type stars.
v1.01: Original distribution

XCLASS: An aid to manual spectral classification

Download source code for XCLASS

xclass.tar.gz

Documentation

xclass.pdf

Standard Spectral Libraries

You will also need to download the same spectral libraries employed by MKCLASS:

mklib.tar.gz