def default_pypeit_par():
"""
Set default parameters for Shane Kast reductions.
"""
par = pypeitpar.PypeItPar()
# Frame numbers
par['calibrations']['standardframe']['number'] = 1
par['calibrations']['biasframe']['number'] = 5
par['calibrations']['pixelflatframe']['number'] = 5
par['calibrations']['traceframe']['number'] = 5
par['calibrations']['arcframe']['number'] = 1
# Scienceimage default parameters
par['scienceimage'] = pypeitpar.ScienceImagePar()
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# 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_exclude_source_objects(monkeypatch):
monkeypatch.setattr(specobjs.SpecObjs, "from_fitsfile", mock_specobjs)
file_list = ['spec1d_file1', 'spec1d_file2']
uncollated_list = SourceObject.build_source_objects(file_list, 'ra/dec')
par = pypeitpar.PypeItPar()
par['collate1d']['exclude_serendip'] = True
par['collate1d']['wv_rms_thresh'] = 0.1
filtered_list, excluded_msgs = exclude_source_objects(
uncollated_list, {'3003': 'Test Exclude`'}, par)
assert [so.spec_obj_list[0].NAME for so in filtered_list
] == ['SPAT1234_SLIT1234_DET01', 'SPAT5334_SLIT4934_DET02']
assert [so.spec1d_file_list[0]
for so in filtered_list] == ['spec1d_file1', 'spec1d_file1']
par['collate1d']['exclude_serendip'] = False
par['coadd1d']['ex_value'] = 'BOX'
par['collate1d']['wv_rms_thresh'] = None
filtered_list, excluded_msgs = exclude_source_objects(
uncollated_list, dict(), par)
assert [so.spec_obj_list[0].NAME for so in filtered_list] == [
'SPAT1234_SLIT1234_DET01', 'SPAT1233_SLIT1235_DET07',
'SPAT6250_SLIT6235_DET03', 'SPAT6256_SLIT6245_DET05',
'SPAT6934_SLIT6245_DET05'
]
assert [so.spec1d_file_list[0] for so in filtered_list] == [
'spec1d_file1', 'spec1d_file1', 'spec1d_file2', 'spec1d_file2',
'spec1d_file2'
]
def default_pypeit_par():
"""
Set default parameters for Keck LRISr reductions.
"""
par = pypeitpar.PypeItPar()
# Set wave tilts order
par['calibrations']['slits']['sigdetect'] = 30.
# 1D wavelengths
par['calibrations']['wavelengths']['rms_threshold'] = 0.20 # Might be grism dependent
# Always sky subtract, starting with default parameters
par['scienceimage'] = pypeitpar.ScienceImagePar()
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# Always correct for flexure, starting with default parameters
par['flexure']['method'] = 'boxcar'
# 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'] = [None, 30] # This may be too low for LRISb
par['calibrations']['traceframe']['exprng'] = [None, 30]
par['scienceframe']['exprng'] = [29, None]
return par
def default_pypeit_par():
"""
Set default parameters for FORS Reductions
"""
par = pypeitpar.PypeItPar()
# Always correct for flexure, starting with default parameters
par['flexure']['method'] = 'boxcar'
# Adjustments to slit and tilts for NIR
par['calibrations']['slits']['sigdetect'] = 50.
par['calibrations']['slits']['trace_npoly'] = 3
par['calibrations']['slits']['maxshift'] = 0.5
# Tilt parameters
par['calibrations']['tilts']['tracethresh'] = 25.0
par['calibrations']['tilts']['spat_order'] = 3
par['calibrations']['tilts']['spec_order'] = 4
# 1D wavelength solution
par['calibrations']['wavelengths']['lamps'] = ['HeI', 'ArI'
] # Grating dependent
par['calibrations']['wavelengths']['rms_threshold'] = 0.25
par['calibrations']['wavelengths']['sigdetect'] = 10.0
par['calibrations']['wavelengths']['fwhm'] = 4.0 # Good for 2x binning
par['calibrations']['wavelengths']['n_final'] = 4
# Flats
par['calibrations']['flatfield']['illumflatten'] = False
par['calibrations']['flatfield']['tweak_slits_thresh'] = 0.90
par['calibrations']['flatfield']['tweak_slits_maxfrac'] = 0.10
return par
def default_pypeit_par():
"""
Set default parameters for Keck LRISb reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'wht_isis_blue'
# Set pixel flat combination method
par['calibrations']['pixelflatframe']['process']['combine'] = 'median'
par['calibrations']['pixelflatframe']['process']['sig_lohi'] = [10.,10.]
# Change the wavelength calibration method
par['calibrations']['wavelengths']['method'] = 'simple'
# Scienceimage default parameters
par['scienceimage'] = pypeitpar.ScienceImagePar()
# Do not flux calibrate
par['fluxcalib'] = None
# 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']['arcframe']['exprng'] = [None, 120]
par['calibrations']['standardframe']['exprng'] = [None, 120]
par['scienceframe']['exprng'] = [90, None]
return par
def default_pypeit_par(self):
"""
Set default parameters for reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'mdm_osmos_mdm4k'
# Ignore PCA
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# Set pixel flat combination method
par['calibrations']['pixelflatframe']['process']['combine'] = 'median'
par['calibrations']['pixelflatframe']['process']['sig_lohi'] = [10.,10.]
# Wavelength calibration methods
par['calibrations']['wavelengths']['method'] = 'full_template'
par['calibrations']['wavelengths']['lamps'] = ['ArI', 'XeI']
par['calibrations']['wavelengths']['reid_arxiv'] = 'mdm_osmos_mdm4k.fits'
par['calibrations']['wavelengths']['sigdetect'] = 10.0
# 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']['arcframe']['exprng'] = [None, None] # Long arc exposures on this telescope
par['calibrations']['standardframe']['exprng'] = [None, 120]
par['scienceframe']['exprng'] = [90, None]
return par
def default_pypeit_par():
"""
Set default parameters for LBT/LUCI reductions.
OLD CODE from LBT MODS
"""
par = pypeitpar.PypeItPar()
# Processing steps
turn_off = dict(use_illumflat=False,
use_biasimage=False,
use_overscan=False,
use_darkimage=False)
par.reset_all_processimages_par(**turn_off)
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_instantiate(fitstbl):
par = pypeitpar.PypeItPar()
spectrograph = load_kast_blue_masters(get_spectrograph=True)[0]
caliBrate = calibrations.MultiSlitCalibrations(fitstbl,
par['calibrations'],
spectrograph)
print(caliBrate)
def default_pypeit_par():
"""
Set default parameters for Keck LRISr reductions.
"""
par = pypeitpar.PypeItPar()
# Set wave tilts order
par['calibrations']['slitedges']['edge_thresh'] = 15.
par['calibrations']['slitedges']['fit_order'] = 3
par['calibrations']['slitedges']['sync_center'] = 'gap'
# TODO: I had to increase this from 1. to 2. to deal with
# Keck_LRIS_red/multi_1200_9000_d680_1x2/ . May need a
# different solution given that this is binned data and most of
# the data in the dev suite is unbinned.
# JXP -- Increased to 6 arcsec. I don't know how 2 (or 1!) could have worked.
par['calibrations']['slitedges']['minimum_slit_length'] = 6
# 1D wavelengths
par['calibrations']['wavelengths']['rms_threshold'] = 0.20 # Might be grism dependent
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# Always correct for flexure, starting with default parameters
par['flexure']['method'] = 'boxcar'
# 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'] = [None, 30] # This may be too low for LRISb
par['calibrations']['traceframe']['exprng'] = [None, 30]
par['scienceframe']['exprng'] = [29, None]
return par
def default_pypeit_par(self):
"""
Set default parameters for magellan MagE reduction.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'magellan_mage'
# Frame numbers
par['calibrations']['standardframe']['number'] = 1
par['calibrations']['biasframe']['number'] = 0
par['calibrations']['pixelflatframe']['number'] = 3
par['calibrations']['traceframe']['number'] = 3
par['calibrations']['arcframe']['number'] = 1
# Bias
par['calibrations']['biasframe']['useframe'] = 'overscan'
# Wavelengths
# 1D wavelength solution
par['calibrations']['wavelengths'][
'rms_threshold'] = 0.20 # Might be grating dependent..
par['calibrations']['wavelengths']['sigdetect'] = 5.0
par['calibrations']['wavelengths']['lamps'] = ['ThAr']
par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[
0]['nonlinear'] * self.detector[0]['saturation']
#par['calibrations']['wavelengths']['method'] = 'reidentify'
# Reidentification parameters
#par['calibrations']['wavelengths']['reid_arxiv'] = 'magellan_thar.json'
par['calibrations']['wavelengths']['ech_fix_format'] = True
# Echelle parameters
par['calibrations']['wavelengths']['echelle'] = True
par['calibrations']['wavelengths']['ech_nspec_coeff'] = 4
par['calibrations']['wavelengths']['ech_norder_coeff'] = 4
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']['order'] = 2
par['calibrations']['tilts']['tracethresh'] = [
10, 10, 10, 10, 10, 10, 10, 10, 10, 10, 10, 10, 10, 10, 10
]
par['calibrations']['slits']['trace_npoly'] = 5
par['calibrations']['slits']['maxshift'] = 3.
par['calibrations']['slits']['pcatype'] = 'order'
# Scienceimage default parameters
par['scienceimage'] = pypeitpar.ScienceImagePar()
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# Do not correct for flexure
par['flexure'] = pypeitpar.FlexurePar()
par['flexure']['method'] = 'skip'
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 20]
par['calibrations']['arcframe']['exprng'] = [20, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
return par
def default_pypeit_par(self):
"""
Set default parameters for Shane Kast Blue reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'keck_nires'
# Frame numbers
par['calibrations']['standardframe']['number'] = 1
par['calibrations']['biasframe']['number'] = 0
par['calibrations']['pixelflatframe']['number'] = 5
par['calibrations']['traceframe']['number'] = 5
par['calibrations']['arcframe']['number'] = 1
# Wavelengths
# 1D wavelength solution
par['calibrations']['wavelengths'][
'rms_threshold'] = 0.20 #0.20 # Might be grating dependent..
par['calibrations']['wavelengths']['sigdetect'] = 5.0
par['calibrations']['wavelengths']['fwhm'] = 5.0
par['calibrations']['wavelengths']['n_final'] = [3, 4, 4, 4, 4]
par['calibrations']['wavelengths']['lamps'] = ['OH_NIRES']
par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[
0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['method'] = 'reidentify'
# Reidentification parameters
par['calibrations']['wavelengths']['reid_arxiv'] = 'keck_nires.fits'
par['calibrations']['wavelengths']['ech_fix_format'] = True
# Echelle parameters
par['calibrations']['wavelengths']['echelle'] = True
par['calibrations']['wavelengths']['ech_nspec_coeff'] = 4
par['calibrations']['wavelengths']['ech_norder_coeff'] = 6
par['calibrations']['wavelengths']['ech_sigrej'] = 3.0
# Tilt parameters
par['calibrations']['tilts']['tracethresh'] = 10.0
#par['calibrations']['tilts']['spat_order'] = 3
#par['calibrations']['tilts']['spec_order'] = 3
# Flats
par['calibrations']['flatfield']['illumflatten'] = False
# Extraction
par['scienceimage']['bspline_spacing'] = 0.8
par['scienceimage']['sn_gauss'] = 4.0
# Flexure
par['flexure']['method'] = 'skip'
par['scienceframe']['process']['sigclip'] = 20.0
par['scienceframe']['process']['satpix'] = 'nothing'
# Overscan but not bias
# This seems like a kludge of sorts
par['calibrations']['biasframe']['useframe'] = 'none'
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 20]
par['calibrations']['arcframe']['exprng'] = [20, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
return par
def default_pypeit_par(self):
"""
Set default parameters for the reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'gemini_flamingos2'
# Image processing steps
turn_off = dict(use_illumflat=False,
use_biasimage=False,
use_overscan=False,
use_darkimage=False)
par.reset_all_processimages_par(**turn_off)
# Wavelengths
# 1D wavelength solution with arc lines
par['calibrations']['wavelengths']['rms_threshold'] = 0.5
par['calibrations']['wavelengths']['sigdetect'] = 5
par['calibrations']['wavelengths']['fwhm'] = 5
par['calibrations']['wavelengths']['n_first'] = 2
par['calibrations']['wavelengths']['n_final'] = 4
par['calibrations']['wavelengths']['lamps'] = ['OH_NIRES']
#par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[0]['nonlinear'] * self.detector[0]['saturation']
#par['calibrations']['wavelengths']['method'] = 'reidentify'
#par['calibrations']['wavelengths']['method'] = 'full_template'
#par['calibrations']['wavelengths']['reid_arxiv'] = 'magellan_fire_long.fits'
par['calibrations']['wavelengths']['match_toler'] = 5.0
# Set slits and tilts parameters
par['calibrations']['tilts']['tracethresh'] = 5
par['calibrations']['tilts']['spat_order'] = 4
par['calibrations']['slitedges']['trace_thresh'] = 10.
par['calibrations']['slitedges']['edge_thresh'] = 200.
#par['calibrations']['slitedges']['det_min_spec_length'] = 0.3
par['calibrations']['slitedges']['fit_min_spec_length'] = 0.4
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 30]
par['calibrations']['tiltframe']['exprng'] = [50, None]
par['calibrations']['arcframe']['exprng'] = [50, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
# Scienceimage parameters
par['reduce']['findobj']['sig_thresh'] = 5.0
par['reduce']['skysub']['sky_sigrej'] = 5.0
par['reduce']['findobj']['find_trim_edge'] = [10, 10]
# Do not correct for flexure
par['flexure']['spec_method'] = 'skip'
# Sensitivity function parameters
par['sensfunc']['algorithm'] = 'IR'
par['sensfunc']['polyorder'] = 8
# ToDo: replace the telluric grid file for Gemini-S site.
par['sensfunc']['IR']['telgridfile'] = resource_filename(
'pypeit',
'/data/telluric/TelFit_LasCampanas_3100_26100_R20000.fits')
return par
def default_pypeit_par():
"""
Set default parameters for Keck LRISb reductions.
"""
par = pypeitpar.PypeItPar()
# Set wave tilts order
par['calibrations']['slits']['sigdetect'] = 20.
par['calibrations']['slits']['trace_npoly'] = 3
# TODO: No longer a parameter
# par['calibrations']['slits']['fracignore'] = 0.02
# par['calibrations']['slits']['pcapar'] = [3,2,1,0]
# 1D wavelength solution
par['calibrations']['wavelengths']['rms_threshold'] = 0.40 # Might be grating dependent..
par['calibrations']['wavelengths']['sigdetect'] = 5. # Doesn't work for reddest chip
par['calibrations']['wavelengths']['lamps'] = ['CuI', 'ArI', 'ArII']
# Overscan subtract the images
#par['calibrations']['biasframe']['useframe'] = 'overscan'
# Alter the method used to combine pixel flats
par['calibrations']['pixelflatframe']['process']['combine'] = 'median'
par['calibrations']['pixelflatframe']['process']['sig_lohi'] = [10.,10.]
# Scienceimage default parameters
par['scienceimage'] = pypeitpar.ScienceImagePar()
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# Always correct for flexure, starting with default parameters
par['flexure'] = pypeitpar.FlexurePar()
# Set the default exposure time ranges for the frame typing
#par['scienceframe']['exprng'] = [30, None]
return par
def default_pypeit_par():
"""
Set default parameters for Shane Kast reductions.
"""
par = pypeitpar.PypeItPar()
# Ignore PCA
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# Flux calibration parset
par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# Always correct for flexure, starting with default parameters
par['flexure']['method'] = 'boxcar'
# 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, 61]
par['calibrations']['standardframe']['exprng'] = [1, 61]
par['scienceframe']['exprng'] = [61, None]
return par
def test_instantiate(fitstbl):
par = pypeitpar.PypeItPar()
spectrograph = load_spectrograph('shane_kast_blue')
caliBrate = calibrations.MultiSlitCalibrations(fitstbl,
par['calibrations'],
spectrograph,
data_path('Masters'))
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 default_pypeit_par(self):
"""
Set default parameters for the reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'gemini_flamingos2'
# No overscan
for key in par['calibrations'].keys():
if 'frame' in key:
par['calibrations'][key]['process']['overscan'] = 'none'
# Wavelengths
# 1D wavelength solution with arc lines
par['calibrations']['wavelengths']['rms_threshold'] = 0.5
par['calibrations']['wavelengths']['sigdetect']=5
par['calibrations']['wavelengths']['fwhm'] = 5
par['calibrations']['wavelengths']['n_first']=2
par['calibrations']['wavelengths']['n_final']=4
par['calibrations']['wavelengths']['lamps'] = ['OH_NIRES']
par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[0]['nonlinear'] * self.detector[0]['saturation']
#par['calibrations']['wavelengths']['method'] = 'reidentify'
#par['calibrations']['wavelengths']['method'] = 'full_template'
#par['calibrations']['wavelengths']['reid_arxiv'] = 'magellan_fire_long.fits'
par['calibrations']['wavelengths']['match_toler']=5.0
# Set slits and tilts parameters
par['calibrations']['tilts']['tracethresh'] = 5
par['calibrations']['tilts']['spat_order'] = 4
par['calibrations']['slitedges']['trace_thresh'] = 10.
par['calibrations']['slitedges']['edge_thresh'] = 200.
#par['calibrations']['slitedges']['det_min_spec_length'] = 0.3
par['calibrations']['slitedges']['fit_min_spec_length'] = 0.4
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# Overscan but not bias
# This seems like a kludge of sorts
par['calibrations']['biasframe']['useframe'] = 'none'
# No overscan
par['scienceframe']['process']['overscan'] ='none'
for key in par['calibrations'].keys():
if 'frame' in key:
par['calibrations'][key]['process']['overscan'] = 'none'
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 30]
par['calibrations']['tiltframe']['exprng'] = [50, None]
par['calibrations']['arcframe']['exprng'] = [50, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
# Scienceimage parameters
#par['reduce']['sig_thresh'] = 5
#par['reduce']['maxnumber'] = 2
par['reduce']['skysub']['sky_sigrej'] = 5.0
par['reduce']['findobj']['find_trim_edge'] = [10,10]
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibratePar()
# Do not correct for flexure
par['flexure'] = None
return par
def default_pypeit_par(self):
"""
Set default parameters for Keck/MOSFIRE
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'keck_mosfire'
# Wavelengths
# 1D wavelength solution
par['calibrations']['wavelengths'][
'rms_threshold'] = 0.20 #0.20 # Might be grating dependent..
par['calibrations']['wavelengths']['sigdetect'] = 5.0
par['calibrations']['wavelengths']['fwhm'] = 5.0
par['calibrations']['wavelengths']['n_final'] = 4
par['calibrations']['wavelengths']['lamps'] = ['OH_NIRES']
par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[
0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['method'] = 'holy-grail'
# Reidentification parameters
#par['calibrations']['wavelengths']['reid_arxiv'] = 'keck_nires.fits'
par['calibrations']['slitedges']['edge_thresh'] = 50.
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# Flats
# Do not illumination correct. We should also not be flat fielding given the bars.
# TODO Implement imaging flats for MOSFIRE. Do test with/without illumination flats.
par['calibrations']['flatfield']['illumflatten'] = False
# Extraction
par['reduce']['skysub']['bspline_spacing'] = 0.8
par['reduce']['extraction']['sn_gauss'] = 4.0
# Flexure
par['flexure']['method'] = 'skip'
par['scienceframe']['process']['sigclip'] = 20.0
par['scienceframe']['process']['satpix'] = 'nothing'
# Overscan but not bias
# This seems like a kludge of sorts
par['calibrations']['biasframe']['useframe'] = 'none'
# No overscan
par['scienceframe']['process']['overscan'] = 'none'
for key in par['calibrations'].keys():
if 'frame' in key:
par['calibrations'][key]['process']['overscan'] = 'none'
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 20]
par['calibrations']['arcframe']['exprng'] = [20, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
# Sensitivity function parameters
par['sensfunc']['algorithm'] = 'IR'
par['sensfunc']['polyorder'] = 8
par['sensfunc']['IR']['telgridfile'] = resource_filename(
'pypeit', '/data/telluric/TelFit_MaunaKea_3100_26100_R20000.fits')
return par
def default_pypeit_par(self):
"""
Set default parameters for magellan MagE reduction.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'magellan_mage'
# Bias
#par['calibrations']['biasframe']['useframe'] = 'overscan'
# Wavelengths
# 1D wavelength solution
par['calibrations']['wavelengths'][
'rms_threshold'] = 0.20 # Might be grating dependent..
par['calibrations']['wavelengths']['sigdetect'] = 5.0
par['calibrations']['wavelengths']['lamps'] = ['ThAr_MagE']
par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[
0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['method'] = 'reidentify'
par['calibrations']['wavelengths']['cc_thresh'] = 0.50
par['calibrations']['wavelengths']['cc_local_thresh'] = 0.50
# Reidentification parameters
par['calibrations']['wavelengths']['reid_arxiv'] = 'magellan_mage.fits'
par['calibrations']['wavelengths']['ech_fix_format'] = True
# Echelle parameters
par['calibrations']['wavelengths']['echelle'] = True
par['calibrations']['wavelengths']['ech_nspec_coeff'] = 4
par['calibrations']['wavelengths']['ech_norder_coeff'] = 4
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'] = [10] * self.norders
par['calibrations']['slitedges']['fit_order'] = 5
par['calibrations']['slitedges']['max_shift_adj'] = 3.
par['calibrations']['slitedges'][
'edge_thresh'] = 10. # Tough to get the bluest orders
par['calibrations']['slitedges']['left_right_pca'] = True
par['calibrations']['slitedges'][
'fit_min_spec_length'] = 0.3 # Allow for a short detected blue order
# Find object parameters
par['scienceimage']['findobj']['find_trim_edge'] = [
4, 4
] # Slit is too short to trim 5,5 especially with 2x binning
# Always flux calibrate, starting with default parameters
par['fluxcalib'] = pypeitpar.FluxCalibrationPar()
# Do not correct for flexure
par['flexure'] = pypeitpar.FlexurePar()
par['flexure']['method'] = 'skip'
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 20]
par['calibrations']['arcframe']['exprng'] = [20, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
return par
def default_pypeit_par():
"""
Set default parameters for KECK HIRES reductions.
"""
par = pypeitpar.PypeItPar()
# Correct for flexure using the default approach
par['flexure'] = pypeitpar.FlexurePar()
return par
def test_sync():
p = pypeitpar.PypeItPar()
proc = pypeitpar.ProcessImagesPar()
proc['combine'] = 'median'
# proc['cr_sigrej'] = 20.5
p.sync_processing(proc)
assert p['scienceframe']['process']['combine'] == 'median'
assert p['calibrations']['biasframe']['process']['combine'] == 'median'
def default_pypeit_par():
"""
Set default parameters for VLT XSHOOTER reductions.
"""
par = pypeitpar.PypeItPar()
# Correct for flexure using the default approach
# par['flexure'] = pypeitpar.FlexurePar()
# Right now turn off flexure compensation
return par
def default_pypeit_par(cls):
"""
Return the default parameters to use for this instrument.
Returns:
:class:`~pypeit.par.pypeitpar.PypeItPar`: Parameters required by
all of ``PypeIt`` methods.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = cls.name
return par
def default_pypeit_par():
"""
Set default parameters for TNG Dolores reductions.
"""
par = pypeitpar.PypeItPar()
# Set the default exposure time ranges for the frame typing
par['calibrations']['biasframe']['exprng'] = [None, 0.1]
par['calibrations']['darkframe']['exprng'] = [999999, None] # No dark frames
par['calibrations']['pinholeframe']['exprng'] = [999999, None] # No pinhole frames
par['scienceframe']['exprng'] = [1, None]
return par
def test_sync():
p = pypeitpar.PypeItPar()
proc = pypeitpar.ProcessImagesPar()
proc['combine'] = 'mean'
proc['sigrej'] = 20.5
p.sync_processing(proc)
assert p['scienceframe']['process']['combine'] == 'mean'
assert p['calibrations']['biasframe']['process']['combine'] == 'mean'
# Sigma rejection of cosmic rays for arc frames is already turned
# off by default
assert p['calibrations']['arcframe']['process']['sigrej'] < 0
assert p['calibrations']['traceframe']['process']['sigrej'] == 20.5
def default_pypeit_par(self):
"""
Set default parameters for Keck LRISb reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'wht_isis_blue'
# Ignore PCA
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# JFH Is this correct?
# Processing steps
turn_off = dict(use_overscan=False)
par.reset_all_processimages_par(**turn_off)
# Turn off the overscan
#for ftype in par['calibrations'].keys():
# try:
# par['calibrations'][ftype]['process']['overscan'] = 'none'
# except (TypeError, KeyError):
# pass
par['scienceframe']['process']['use_overscan'] = False
# Make a bad pixel mask
par['calibrations']['bpm_usebias'] = True
# Set pixel flat combination method
par['calibrations']['pixelflatframe']['process']['combine'] = 'median'
par['calibrations']['pixelflatframe']['process']['sig_lohi'] = [
10., 10.
]
# Change the wavelength calibration method
par['calibrations']['wavelengths']['method'] = 'full_template'
par['calibrations']['wavelengths']['lamps'] = [
'NeI', 'ArI', 'ArII', 'CuI'
]
#par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['n_first'] = 3
par['calibrations']['wavelengths']['n_final'] = 5
par['calibrations']['wavelengths']['sigdetect'] = 10.0
par['calibrations']['wavelengths']['wv_cen'] = 4859.0
par['calibrations']['wavelengths']['disp'] = 0.2
# Do not flux calibrate
par['fluxcalib'] = None
# 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']['arcframe']['exprng'] = [None, 120]
par['calibrations']['standardframe']['exprng'] = [None, 120]
par['scienceframe']['exprng'] = [90, None]
return par
def default_pypeit_par(self):
"""
Set default parameters for MMT/BINOSPEC reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'mmt_binospec'
# Frame numbers
par['calibrations']['standardframe']['number'] = 0
par['calibrations']['biasframe']['number'] = 0
par['calibrations']['pixelflatframe']['number'] = 5
par['calibrations']['traceframe']['number'] = 5
par['calibrations']['arcframe']['number'] = 5
par['calibrations']['arcframe']['process']['overscan'] = 'median'
# Wavelengths
# 1D wavelength solution
par['calibrations']['wavelengths']['rms_threshold'] = 0.5
par['calibrations']['wavelengths']['sigdetect'] = 20.
par['calibrations']['wavelengths']['fwhm'] = 5.0
par['calibrations']['wavelengths']['lamps'] = ['ArI', 'ArII']
par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[
0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['method'] = 'holy-grail'
# Tilt and slit parameters
par['calibrations']['tilts']['tracethresh'] = 10.0
par['calibrations']['tilts']['spat_order'] = 6
par['calibrations']['tilts']['spec_order'] = 6
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# Flats
par['calibrations']['flatfield']['illumflatten'] = True
# Extraction
par['reduce']['skysub']['bspline_spacing'] = 0.8
par['reduce']['extraction']['sn_gauss'] = 4.0
## Do not perform global sky subtraction for standard stars
## FW: The slit is too wide and the target usually close to the center where is the boundary
## two detectors. global_sky will cause some problem sometime.
par['reduce']['skysub']['global_sky_std'] = False
# Flexure
par['flexure']['method'] = 'skip'
par['scienceframe']['process']['sigclip'] = 20.0
par['scienceframe']['process']['satpix'] = 'nothing'
#par['scienceframe']['process']['overscan'] ='median'
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 100]
par['calibrations']['arcframe']['exprng'] = [20, None]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
return par
def default_pypeit_par(self):
"""
Set default parameters for Keck/MOSFIRE
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'lbt_luci2'
# for key in par['calibrations'].keys():
# print(key)
# par['calibrations'][key]['process']['overscan'] = 'none'
# Wavelengths
# 1D wavelength solution
par['calibrations']['wavelengths'][
'rms_threshold'] = 0.20 # 0.20 # Might be grating dependent..
par['calibrations']['wavelengths']['sigdetect'] = 5.0
par['calibrations']['wavelengths']['fwhm'] = 5.0
par['calibrations']['wavelengths']['n_final'] = 4
par['calibrations']['wavelengths']['lamps'] = ['OH_NIRES']
par['calibrations']['wavelengths']['nonlinear_counts'] = \
self.detector[0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['method'] = 'holy-grail'
par['calibrations']['slitedges']['edge_thresh'] = 300
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
par['calibrations']['slitedges']['fit_order'] = 8
# Flats
par['calibrations']['flatfield']['illumflatten'] = True
# par['calibration']['flatfield']['tweak_slits'] = False
# Extraction
# Model full slit currently turned on
par['reduce']['extraction']['model_full_slit'] = True
# Tailored profile nsigma parameter for the standard
par['reduce']['extraction']['std_prof_nsigma'] = 100.
# Do not perform global sky subtraction for standard stars
par['reduce']['skysub']['global_sky_std'] = False
par['reduce']['skysub']['bspline_spacing'] = 0.8
par['reduce']['extraction']['sn_gauss'] = 4.0
# Flexure
par['flexure']['method'] = 'skip'
par['scienceframe']['process']['sigclip'] = 20.0
par['scienceframe']['process']['satpix'] = 'nothing'
# par['scienceframe']['process']['satpix'] = 'reject'
par['scienceframe']['process']['overscan'] = 'none'
# par['standardframe']['process']['overscan'] = 'none'
return par
def default_pypeit_par(self):
"""
Set default parameters for Gemini GNIRS reductions.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'gemini_gnirs'
# Image processing steps
turn_off = dict(use_illumflat=False,
use_biasimage=False,
use_overscan=False,
use_darkimage=False)
par.reset_all_processimages_par(**turn_off)
# Flats
par['calibrations']['flatfield']['tweak_slits_thresh'] = 0.90
par['calibrations']['flatfield']['tweak_slits_maxfrac'] = 0.10
# Reduce parameters
par['reduce']['findobj'][
'sig_thresh'] = 5.0 # Object finding threshold
par['reduce']['findobj']['find_trim_edge'] = [
2, 2
] # Slit is too short to trim 5,5 especially
par['reduce']['findobj'][
'find_cont_fit'] = False # Don't continuum fit objfind for narrow slits
par['reduce']['findobj'][
'find_npoly_cont'] = 0 # Continnum order for determining thresholds
par['reduce']['skysub']['bspline_spacing'] = 0.8
par['reduce']['skysub'][
'global_sky_std'] = False # Do not perform global sky subtraction for standard stars
par['reduce']['skysub'][
'no_poly'] = True # Do not use polynomial degree of freedom for global skysub
par['reduce']['extraction'][
'model_full_slit'] = True # local sky subtraction operates on entire slit
# Do not correct for flexure
par['flexure']['spec_method'] = 'skip'
# Set the default exposure time ranges for the frame typing
par['calibrations']['pixelflatframe']['exprng'] = [None, 30]
par['calibrations']['traceframe']['exprng'] = [None, 30]
par['calibrations']['standardframe']['exprng'] = [None, 30]
par['scienceframe']['exprng'] = [30, None]
# Sensitivity function parameters
par['sensfunc']['algorithm'] = 'IR'
par['sensfunc']['polyorder'] = 8
par['sensfunc']['IR']['telgridfile'] = resource_filename(
'pypeit', '/data/telluric/TelFit_MaunaKea_3100_26100_R20000.fits')
return par
def default_pypeit_par(self):
"""
Set default parameters.
"""
par = pypeitpar.PypeItPar()
par['rdx']['spectrograph'] = 'magellan_fire_long'
# Wavelengths
# 1D wavelength solution with arc lines
par['calibrations']['wavelengths']['rms_threshold'] = 1.0
par['calibrations']['wavelengths']['sigdetect'] = 3
par['calibrations']['wavelengths']['fwhm'] = 20
par['calibrations']['wavelengths']['n_first'] = 2
par['calibrations']['wavelengths']['n_final'] = 4
par['calibrations']['wavelengths']['lamps'] = [
'ArI', 'ArII', 'ThAr', 'NeI'
]
#par['calibrations']['wavelengths']['nonlinear_counts'] = self.detector[0]['nonlinear'] * self.detector[0]['saturation']
par['calibrations']['wavelengths']['method'] = 'full_template'
par['calibrations']['wavelengths'][
'reid_arxiv'] = 'magellan_fire_long.fits'
par['calibrations']['wavelengths']['match_toler'] = 5.0
# Set slits and tilts parameters
par['calibrations']['tilts']['tracethresh'] = 5
par['calibrations']['slitedges']['trace_thresh'] = 10.
par['calibrations']['slitedges']['sync_predict'] = 'nearest'
# Processing steps
turn_off = dict(use_illumflat=False,
use_biasimage=False,
use_overscan=False,
use_darkimage=False)
par.reset_all_processimages_par(**turn_off)
# Scienceimage parameters
par['reduce']['findobj']['sig_thresh'] = 5
#par['reduce']['maxnumber'] = 2
par['reduce']['findobj']['find_trim_edge'] = [50, 50]
par['flexure']['spec_method'] = 'skip'
par['sensfunc']['IR']['telgridfile'] = resource_filename(
'pypeit',
'/data/telluric/TelFit_LasCampanas_3100_26100_R20000.fits')
# Set the default exposure time ranges for the frame typing
par['calibrations']['standardframe']['exprng'] = [None, 60]
par['calibrations']['arcframe']['exprng'] = [1, 50]
par['calibrations']['darkframe']['exprng'] = [20, None]
par['scienceframe']['exprng'] = [20, None]
return par
