# File: sof/gravity_vis/350.gravity_vis.calibrator_HIGH_COMBINED_COMBINED/gravity_vis.rc
#
# Note: This configuration file has been automatically
#       generated by the esorex (v3.14a) program.
#
# Date: 28-Jul-2026 13:32:27
#
#

# --static-name
# Use static names for the products (for ESO).
gravity.dfs.static-name=FALSE

# --bias-subtracted-file
# Save the BIAS_SUBTRACTED intermediate product.
gravity.dfs.bias-subtracted-file=FALSE

# --spectrum-file
# Save the SPECTRUM intermediate product.
gravity.dfs.spectrum-file=FALSE

# --preproc-file
# Save the PREPROC intermediate product.
gravity.dfs.preproc-file=FALSE

# --p2vmreduced-file
# Save the P2VMRED intermediate product.
gravity.dfs.p2vmred-file=FALSE

# --astro-file
# Save the ASTROREDUCED intermediate product.
gravity.dfs.astro-file=FALSE

# --flatten-visphi
# Use the PCA calibrator to flatten the VISPHI.
gravity.vis.flatten-visphi=FALSE

# --average-vis
# Average the results from the different input files (if any)
# in the output product, instead of simply appending them.
gravity.postprocess.average-vis=FALSE

# --bias-method
# Method to average the biaspixels when cleaning-up
# the SC detector (only applied to MED and LOW). Ideally
# the same value shall be used when reducing the DARK
# with gravity_dark and the OBJECT with gravity_vis. 
# UTO is equivalent to MASKED_MEDIAN_PER_COLUMN if the data
# ontains in the IMAGING_DETECTOR_SC extension the
# EFT, HALFLEFT, CENTER, HALFRIGHT and RIGHT columns.
# therwise it is like MEDIAN. <AUTO | MEDIAN | MEDIAN_PER_COLUMN |
# MASKED_MEDIAN_PER_COLUMN>
gravity.preproc.bias-method=AUTO

# --remove-cosmicrays
# Remove the cosmicrays with the statiscal method.
gravity.preproc.remove-cosmicrays=TRUE

# --acq-correction-delay
# Delay between the end of ACQ frame and correction
# offset seen by the metrology diodes, in seconds.
gravity.metrology.acq-correction-delay=0.25

# --use-fiber-dxy
# Use the fiber position when computing OPD_TEL_CORR.
gravity.metrology.use-fiber-dxy=FALSE

# --use-met-rtc
# Reduce metrology voltage with the real time algorithm
# nstead of using the pipeline’s algorithm.
gravity.metrology.use-met-rtc=FALSE

# --use-faint-met
# In FAINT also the faint parts of the metrology 
# re used, not only the bright periods.
gravity.metrology.use-faint-met=TRUE

# --preswitch-delay
# Delay where metrology values are ignored before
# aser brightness is switched in faint mode, ms.
gravity.metrology.preswitch-delay=60

# --postswitch-delay
# Delay where metrology values are ignored after
# aser brightness is switched in faint mode, ms.
gravity.metrology.postswitch-delay=320

# --demodulate-metrology
# Perform demodulation on the raw metrology data.
gravity.metrology.demodulate-metrology=TRUE

# --use-dark-offsets
# Use diode zeros measured from the DARK when demodulating metrology.
gravity.metrology.use-dark-offsets=TRUE

# --chi2r-threshold
# Threshold in chi2r of the fringe-fit to declare
# a bad value. This is usefull to detect outliers
# or cosmic in individual frames.
gravity.signal.chi2r-threshold=50.0

# --chi2r-sigma
# Threshold in chi2r of the fringe-fit (in unit of the 
# the std of chi2r in the spectral direction) to declare
# a bad value. This is usefull to detect outliers
# or cosmic in individual frames.
gravity.signal.chi2r-sigma=100.0

# --nsmooth-snr-ft
# Number of samples to average coherently when computing
# the real-time SNR and GDELAY of the FT (shall correspond
# to the atmospheric coherence time). The integration
# window runs from -nsmooth -> +nsmooth.
gravity.signal.nsmooth-snr-ft=5

# --phase-ref-sc-maxdeg
# Maximum deg for the fit of PHASE_REF.
gravity.signal.phase-ref-sc-maxdeg=3

# --use-met-zero
# Flag to add a constant value to OPD_DISP.
# This constant value is taken from the header.
gravity.signal.use-met-zero=FALSE

# --imaging-ref-met
# Metrology source used for IMAGING_REF calculation:
# Use fibre coupler metrology (FC);
# Use fibre coupler metrology corrected from pupil motion (FC_CORR);
# Use telescope metrology (TEL). <FC | FC_CORR | TEL>
gravity.signal.imaging-ref-met=FC

# --snr-min-ft
# SNR threshold to accept FT frames (>0). It raises the first bit (<<0)
# of column REJECTION_FLAG of FT.
gravity.signal.snr-min-ft=3.0

# --global-state-min-ft
# Minimum OPDC state to accept FT frames (>=0) It raises the second bit
# (<<1) of column REJECTION_FLAG of FT.
gravity.signal.global-state-min-ft=2.0

# --global-state-max-ft
# Maximum OPDC state to accept FT frames (>=0) It raises the second bit
# (<<1) of column REJECTION_FLAG of FT.
gravity.signal.global-state-max-ft=4.0

# --state-min-ft
# Minimum OPDC state per baseline to accept FT frames (>=0) It raises
# the second bit (<<1) of column REJECTION_FLAG of FT.
gravity.signal.state-min-ft=1.0

# --tracking-min-sc
# Minimum ratio of accepted FT frames in order to accept a SC frames (0..1),
# that is, for each SC DIT, the fraction of the time the
# REJECTION_FLAG of the FT is not 0.
# It raises the first bit (<<0) of column REJECTION_FLAG of SC.
gravity.signal.tracking-min-sc=0.8

# --vfactor-min-sc
# vFactor threshold to accept SC frame (0..1).
gravity.signal.vfactor-min-sc=0.1

# --opd-pupil-max-sc
# Maximum OPD_PUPIL (abs) to accept SC frames. It raises the third bit
# (<<2) of column REJECTION_FLAG of SC.
gravity.signal.opd-pupil-max-sc=9999.0

# --opd-pupil-stddev-max-sc
# Maximum OPD_PUPIL_STDDEV to accept SC frames. It
# raises the fourth bit (<<3) of REJECTION_FLAG of SC.
gravity.signal.opd-pupil-stddev-max-sc=2.9e-07

# --max-frame
# Maximum number of frames to integrate 
# coherently into an OIFITS entry.
gravity.vis.max-frame=10000

# --force-same-time
# Force all baseline/quantities to have
# strictly the same TIME and MJD columns.
gravity.vis.force-same-time=FALSE

# --debias-sc
# Subtract the V2 bias from SC.
gravity.vis.debias-sc=TRUE

# --debias-ft
# Subtract the V2 bias from FT.
gravity.vis.debias-ft=TRUE

# --nboot
# Number of bootstraps to compute error (1..100).
gravity.vis.nboot=20

# --vis-correction-sc
# Correction of SC visibility from losses due to long integration,
# using the measured visibility losses with the FT (VFACTOR
# and/or PFACTOR) or by forcing
# the SC visibilities to match those of the FT (FORCE). Possible
# choices are:. <VFACTOR | PFACTOR | VFACTOR_PFACTOR | FORCE | NONE>
gravity.vis.vis-correction-sc=VFACTOR

# --vis-correction-ft
# Correction of FT visibility from losses due to long integration,
# using a sliding window P_FACTOR, or its square. Choices are:. <NONE |
# PFACTOR | PFACTOR_SQUARED>
gravity.vis.vis-correction-ft=NONE

# --pfactor-window-length
# Length of the sliding window used to calculate the FT P_FACTOR.
# For each FT frame, the window will run from -window-length to
# +window-length inclusive.
gravity.vis.pfactor-window-length=40

# --phase-ref-sc
# Reference phase used to integrate the SC frames.
# Use a self-estimate of the phase, fitted by poly. (SELF_REF)
# Use the FT phase only, interpolated in lbd (PHASE_REF)
# Use the FT+MET-SEP.UV phase (IMAGING_REF). <SELF_REF | PHASE_REF |
# IMAGING_REF | AUTO | NONE>
gravity.vis.phase-ref-sc=AUTO

# --output-phase-sc
# With DIFFERENTIAL, the mean group-delay and mean
# phases are removed from the output VISPHI in the
# final OIFITS file. With ABSOLUTE, the VISPHI is
# kept unmodified. With SELF_VISPHI, the internal differential
# phase between each spectral channel and a common 
# reference channel is computed. <DIFFERENTIAL | ABSOLUTE | AUTO |
# SELF_VISPHI>
gravity.vis.output-phase-sc=AUTO

# --output-phase-channels
# range (string in the form [min,max]) of channels
# to use a SELF_VISPHI phase reference.
gravity.vis.output-phase-channels=[0,0]

# --outlier-fraction-threshold
# Flag channels with more than this fraction of the frames
# affected by outliers or cosmics. These are typically detected
# with the thresholds options in chi2 of the fringe-fit.
gravity.vis.outlier-fraction-threshold=0.5

# --flat-flux
# Normalize the flux (stored in OI_FLUX binary extension) with instrument
# transmission recorded in the 
# nput P2VM calibration map. Consequently, the flux quantity is either the
# intensity level recorded 
# n the detector, thus including the instrument transmission (FALSE); or the
# intensity level at the instrument entrance (TRUE).
gravity.vis.flat-flux=FALSE

# --average-sky
# Average the SKYs into a master SKY. If FALSE, the recipe loops
# over the SKY to reduce each OBJECT with a different SKY.
gravity.preproc.average-sky=FALSE

# --reduce-acq-cam
# If TRUE, reduced ACQ_CAM images. If QC, compute only
# the QC parameters of the field part. If FALSE, ignore
# completely the acquisition camera. <TRUE | true | FALSE | false | QC | qc>
gravity.test.reduce-acq-cam=FALSE

# --color-wave-correction
# If TRUE, creates a new OI_WAVELENGTH_EFF with corrected wavelength.
gravity.vis.color-wave-correction=FALSE

# --oifits2
# If TRUE, the output products will be fully OIFITS2 compliant. Note that TRUE
# will be the default and eventually the parameter will be removed in the
# future.
gravity.vis.oifits2=TRUE

#
# End of file