def default_pypeit_par():
"""
Set default parameters for LBT/LUCI reductions.
OLD CODE from LBT MODS
"""
par = pypeitpar.PypeItPar()
# Scienceimage default parameters
par['reduce'] = pypeitpar.ReducePar()
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibratePar()
# Always correct for flexure, starting with default parameters
par['flexure'] = pypeitpar.FlexurePar()
# Set the default exposure time ranges for the frame typing
par['calibrations']['biasframe']['exprng'] = [None, 1]
par['calibrations']['darkframe']['exprng'] = [999999,
None] # No dark frames
par['calibrations']['pinholeframe']['exprng'] = [999999, None
] # No pinhole frames
par['calibrations']['pixelflatframe']['exprng'] = [0, None]
par['calibrations']['traceframe']['exprng'] = [0, None]
par['calibrations']['arcframe']['exprng'] = [None, 60]
par['calibrations']['standardframe']['exprng'] = [1, 200]
par['scienceframe']['exprng'] = [200, None]
return par
def test_reduce():
pypeitpar.ReducePar()
def default_pypeit_par(self):
"""
Set default parameters for Shane Kast Blue reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'magellan_fire'
# No overscan
for key in par['calibrations'].keys():
if 'frame' in key:
par['calibrations'][key]['process']['overscan'] = 'none'
# Wavelengths
# 1D wavelength solution with OH lines
par['calibrations']['wavelengths']['rms_threshold'] = 1.0
par['calibrations']['wavelengths']['sigdetect'] = [
5, 10, 10, 10, 10, 20, 30, 30, 30, 30, 30, 10, 30, 30, 60, 30, 30,
10, 20, 30, 10
]
par['calibrations']['wavelengths']['n_first'] = 2
par['calibrations']['wavelengths']['n_final'] = [
3, 3, 3, 2, 4, 4, 4, 3, 4, 4, 4, 3, 4, 4, 4, 4, 4, 4, 6, 6, 4
]
par['calibrations']['wavelengths']['lamps'] = ['OH_FIRE_Echelle']
par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[
0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['method'] = 'reidentify'
par['calibrations']['wavelengths']['cc_thresh'] = 0.35
par['calibrations']['wavelengths'][
'reid_arxiv'] = 'magellan_fire_echelle.fits'
par['calibrations']['wavelengths']['match_toler'] = 30.0
# Echelle parameters
par['calibrations']['wavelengths']['echelle'] = True
par['calibrations']['wavelengths']['ech_fix_format'] = True
par['calibrations']['wavelengths']['ech_nspec_coeff'] = 4
par['calibrations']['wavelengths']['ech_norder_coeff'] = 6
par['calibrations']['wavelengths']['ech_sigrej'] = 3.0
# Always correct for flexure, starting with default parameters
par['flexure'] = pypeitpar.FlexurePar()
par['scienceframe']['process']['sigclip'] = 20.0
par['scienceframe']['process']['satpix'] = 'nothing'
# Set slits and tilts parameters
par['calibrations']['tilts']['tracethresh'] = 5
par['calibrations']['slitedges']['edge_thresh'] = 10.
par['calibrations']['slitedges']['trace_thresh'] = 10.
par['calibrations']['slitedges']['fit_order'] = 5
par['calibrations']['slitedges']['max_shift_adj'] = 0.5
par['calibrations']['slitedges']['fit_min_spec_length'] = 0.5
par['calibrations']['slitedges']['left_right_pca'] = True
par['calibrations']['slitedges']['pca_order'] = 3
# Scienceimage default parameters
par['reduce'] = pypeitpar.ReducePar()
# Always flux calibrate, starting with default parameters
#par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# Do not correct for flexure
par['flexure'] = None
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 60]
par['calibrations']['arcframe']['exprng'] = [20, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
# Sensitivity function parameters
# Sensitivity function parameters
par['sensfunc']['algorithm'] = 'IR'
par['sensfunc']['polyorder'] = 8
# place holder for telgrid file
par['sensfunc']['IR']['telgridfile'] = resource_filename(
'pypeit', '/data/telluric/TelFit_MaunaKea_3100_26100_R20000.fits')
return par