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Table 1.

Overview of all switches and parameters in the main configuration file of the GIST pipeline.

Config-Switch Brief description
Main switches
DEBUG Runs pipeline on one central line of pixels
VORONOI Performs Voronoi-binning on the data prior to the analysis
GANDALF Runs the GANDALF module (pyGandALF) on bins or spaxels
SFH Runs the SFH module (regularised pPXF)
LINE_STRENGTH Runs the LS module
PARALLEL Activates multiprocessing
NCPU Number of cores to use for multiprocessing

General settings
RUN_NAME Name of the analysis run
IFU Identifier of the read-in routine
LMIN Minimum rest-frame wavelength [Å]
LMAX Maximum rest-frame wavelength [Å]
ORIGIN Origin of the coordinate system [arcsec]
REDSHIFT Redshift of the system [z]
SIGMA Initial guess of velocity dispersion [km s−1]
TARGET_SNR Target signal-to-noise ratio for the binning
MIN_SNR Minimum signal-to-noise ratio per spaxel to be accepted for the Voronoi binning
COVAR_VOR Corrects for spatial correlations of the noise in the Voronoi binning process
SSP_LIB Defines the spectral template library
NORM_TEMP Normalises the spectral template library to obtain light- or mass-weighted results

PPXF settings
MOM Number of kinematic moments
ADEG Degree of the add. Legendre polynomial
MDEG Degree of the mult. Legendre polynomial
MC_PPXF Number of Monte Carlo simulations used to extract errors on the stellar kinematics

GANDALF settings
FOR_ERRORS Derives errors on the emission-lines
REDDENING Includes the effect of reddening by dust
EBmV De-reddens the spectra for the Galactic extinction in the direction of the target

SFH settings
REGUL_ERR Regularisation error (reciprocal of the pPXF keyword “REGUL”)
FIXED Fixes stellar kinematics to the results obtained with the PPXF module (See correspondent pPXF keyword)
NOISE Passes a constant noise vector to pPXF

Line strength settings
CONV_COR Resolution of the index measurement [Å]
MC_LS Number of Monte Carlo simulations used to extract errors on the LS indices

SSP settings
NWALKER Number of walkers for the MCMC algorithm (used for the conversion of indices to population properties)
NCHAIN Number of iterations in the MCMC algorithm (used for the conversion of indices to population properties)

Notes. This file contains one line per galaxy in consideration.

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