def __init__(self, epoch, field, filt, rootDir='/u/ghezgroup/data/gc/',
epochDirSuffix=None, useDistorted=False, cleanList='c.lis'):
"""
For Arches reduction:
epoch -- '06maylgs' for example
field -- 'f1', 'f2', etc. This sets the PSF star list to use.
filt -- 'kp', 'lp', or 'h'
"""
# Setup some Arches specific parameters
self.mapFilter2Cal = {'kp': 1, 'h': 2, 'lp': 3}
self.mapField2CooStar = {'arch_f1': 'f1_psf0',
'arch_f2': 'f2_psf8',
'arch_f3': 'f3_psf0',
'arch_f4': 'f4_psf0',
'arch_f5': 'f5_psf1',
'arch_f6': 'f6_psf7'}
self.mapField2CalStars = {'arch_f1': ['f1_psf0', 'f1_psf1', 'f1_psf2', 'f1_psf3', 'f1_psf4', 'f1_psf5', 'f1_psf6', 'f1_psf7','f1_psf9'],
'arch_f2': ['f2_psf0', 'f2_psf2', 'f2_psf3', 'f2_psf4', 'f2_psf6', 'f2_psf7', 'f2_psf8', 'f2_psf9', 'f2_psf10', 'f2_psf11', 'f2_psf12', 'f2_psf13'],
'arch_f3': ['f3_psf0', 'f3_psf1', 'f3_psf5'],
'arch_f4': ['f4_psf0', 'f4_psf2'],
'arch_f5': ['f5_psf0', 'f5_psf1', 'f5_psf2', 'f5_psf3', 'f5_psf4', 'f5_psf5', 'f5_psf12'],
'arch_f6': ['f6_psf2', 'f6_psf3'],
}
# Initialize the Analysis object
Analysis.__init__(self, epoch, filt=field + '_' + filt,
rootDir=rootDir, epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted, cleanList=cleanList)
# Use the field to set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'arches/psfstars/%s_%s_psf_all.list' % \
(field, filt)
##########
# Setup the appropriate calibration stuff.
##########
# By default use the first 10 PSF stars.
self.calStars = self.mapField2CalStars[field]
# Choose the column based on the filter
self.calColumn = self.mapFilter2Cal[filt]
# Set the coo star
self.cooStar = self.mapField2CooStar[field]
self.calCooStar = self.cooStar
# Override some of the default parameters
# self.calFlags = '-f 1 -c 4 -R '
self.calFlags = '-f 1 -R '
self.calFile = '/u/ghezgroup/data/gc/source_list/photo_calib_arch.dat'
self.labellist = '/u/ghezgroup/data/gc/source_list/label_arch.dat'
self.orbitlist = None
def __init__(self,
epoch,
field,
filt,
rootDir='/u/ghezgroup/data/gc/',
epochDirSuffix=None,
useDistorted=False,
cleanList='c.lis'):
"""
For Quintuplet reduction:
epoch -- '06maylgs' for example
field -- 'f1', etc. This sets the PSF star list to use.
filt -- 'kp'
"""
# Setup some Arches specific parameters
self.mapFilter2Cal = {'kp': 1}
self.mapField2CooStar = {'quint_f1': 'psf0'}
# Initialize the Analysis object
Analysis.__init__(self,
epoch,
filt=field + '_' + filt,
rootDir=rootDir,
epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted,
cleanList=cleanList)
# Use the field to set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'quintuplet/psfstars/%s_%s_psf.list' % \
(field, filt)
# Setup the appropriate calibration stuff.
# By default use the first 10 PSF stars.
self.calStars = ['psf0', 'psf1', 'psf2', 'psf4']
# Choose the column based on the filter
self.calColumn = self.mapFilter2Cal[filt]
# Set the coo star
self.cooStar = self.mapField2CooStar[field]
self.calCooStar = self.cooStar
# Override some of the default parameters
# self.calFlags = '-f 1 -c 4 -R '
self.calFlags = '-f 1 -R '
self.calFile = '/u/ghezgroup/data/gc/source_list/photo_calib_quint.dat'
self.labellist = '/u/ghezgroup/data/gc/source_list/label_quint.dat'
self.orbitlist = None
def __init__(self, epoch, rootDir='/u/ghezgroup/data/gc/'):
"""
For Speckle reduction:
epoch -- '02apr' for example
filt -- must use '' because the filt is not specified in image names
"""
# Initialize the Analysis object
Analysis.__init__(self, epoch, filt='', rootDir=rootDir, cleanList=None)
# Set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'gc/starfinder/psfstars/psf_central.dat'
# Override some of the default parameters
self.type = 'speckle'
# self.calFlags = '-f 1 -c 1 -R '
self.calFlags = '-f 1 -R '
def __init__(self, epoch, field, filt, rootDir='/u/ghezgroup/data/gc/',
epochDirSuffix=None, useDistorted=False, cleanList='c.lis'):
"""
For Quintuplet reduction:
epoch -- '06maylgs' for example
field -- 'f1', etc. This sets the PSF star list to use.
filt -- 'kp'
"""
# Setup some Arches specific parameters
self.mapFilter2Cal = {'kp': 1}
self.mapField2CooStar = {'quint_f1': 'psf0'}
# Initialize the Analysis object
Analysis.__init__(self, epoch, filt=field + '_' + filt,
rootDir=rootDir, epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted, cleanList=cleanList)
# Use the field to set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'quintuplet/psfstars/%s_%s_psf.list' % \
(field, filt)
# Setup the appropriate calibration stuff.
# By default use the first 10 PSF stars.
self.calStars = ['psf0', 'psf1', 'psf2', 'psf4']
# Choose the column based on the filter
self.calColumn = self.mapFilter2Cal[filt]
# Set the coo star
self.cooStar = self.mapField2CooStar[field]
self.calCooStar = self.cooStar
# Override some of the default parameters
# self.calFlags = '-f 1 -c 4 -R '
self.calFlags = '-f 1 -R '
self.calFile = '/u/ghezgroup/data/gc/source_list/photo_calib_quint.dat'
self.labellist = '/u/ghezgroup/data/gc/source_list/label_quint.dat'
self.orbitlist = None
def __init__(self,
epoch,
filt,
rootDir='/g/lu/data/orion/2010oct/',
epochDirSuffix=None,
useDistorted=False,
cleanList='c.lis'):
"""
For reduction of deep wide mosaics:
epoch -- '06maylgs1' for example
filt -- 'dp_msc_C_kp', 'dp_msc_NE_kp', 'dp_msc_SE_kp', and so on...
"""
# Create dictionary which maps the PSF stars to the field
self.mapFilter2CalStars = {
'orion_msc_a_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374'],
'orion_msc_b_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1366'],
'orion_msc_c_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1366'],
'orion_msc_d_kp':
['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366', 'ir1486'],
'orion_msc_e_kp':
['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_f_kp':
['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_g_kp':
['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_h_kp':
['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_i_kp':
['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_j_kp':
['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'BN_Mosaic_A_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1486',
'ir1519', 'toller_5', 'toller_6', 'toller_7', 'toller_8',
'toller_9', 'toller_10', 'CXOONC'
],
'BN_Mosaic_B_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1486',
'ir1519', 'toller_5', 'toller_6', 'toller_7', 'toller_8',
'toller_9', 'toller_10', 'CXOONC'
],
'BN_Mosaic_C_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1486',
'toller_6', 'toller_7', 'toller_8', 'toller_9', 'CXOONC',
'toller_10', 'toller_5', 'ir1519'
],
'BN_Mosaic_D_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1486', 'toller_5',
'toller_6', 'toller_7', 'toller_8', 'toller_9', 'CXOONC',
'toller_10', 'toller_3'
],
'BN_Mosaic_E_kp': [
'Pare1839', 'ir1491', 'ir1486', 'toller_8', 'toller_9',
'toller_3', 'toller_2', 'toller_4', 'toller_11', 'toller_12',
'toller_13'
],
'BN_Mosaic_F_kp': [
'toller_4', 'toller_2', 'toller_3', 'toller_11', 'toller_12',
'toller_13'
],
'BN_Mosaic_G_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1486', 'toller_5',
'toller_6', 'toller_7', 'toller_8', 'toller_9', 'toller_2',
'toller_3', 'CXOONC'
],
'BN_Mosaic_H_kp': [
'IRn', 'Pare1839', 'ir1374', 'ir1352', 'ir1486', 'toller_8',
'CXOONC', 'toller_10'
],
'BN_Mosaic_I_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'CXOONC',
'toller_5', 'toller_6', 'toller_7', 'toller_9'
],
'BN_Mosaic_J_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1519',
'ir1486', 'CXOONC', 'toller_5', 'toller_6', 'toller_7',
'toller_8', 'toller_9', 'toller_10'
],
'BN_Mosaic_K_kp': [
'IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1519',
'ir1486', 'CXOONC', 'toller_5', 'toller_6', 'toller_7',
'toller_8', 'toller_9', 'toller_10'
],
}
self.mapFilter2Coo = {
'orion_msc_a_kp': 'IRn',
'orion_msc_b_kp': 'IRn',
'orion_msc_c_kp': 'IRn',
'orion_msc_d_kp': 'IRn',
'orion_msc_e_kp': 'IRn',
'orion_msc_f_kp': 'IRn',
'orion_msc_g_kp': 'IRn',
'orion_msc_h_kp': 'IRn',
'orion_msc_i_kp': 'IRn',
'orion_msc_j_kp': 'IRn',
'BN_Mosaic_A_kp': 'Pare1839',
'BN_Mosaic_B_kp': 'Pare1839',
'BN_Mosaic_C_kp': 'Pare1839',
'BN_Mosaic_D_kp': 'Pare1839',
'BN_Mosaic_E_kp': 'ir1491',
'BN_Mosaic_F_kp': 'toller_4',
'BN_Mosaic_G_kp': 'Pare1839',
'BN_Mosaic_H_kp': 'Pare1839',
'BN_Mosaic_I_kp': 'ir1374',
'BN_Mosaic_J_kp': 'Pare1839',
'BN_Mosaic_K_kp': 'Pare1839',
}
self.mapFilter2CalCoo = {
'orion_msc_a_kp': 'IRn',
'orion_msc_b_kp': 'IRn',
'orion_msc_c_kp': 'ir1374',
'orion_msc_d_kp': 'IRn',
'orion_msc_e_kp': 'IRn',
'orion_msc_f_kp': 'IRn',
'orion_msc_g_kp': 'IRn',
'orion_msc_h_kp': 'IRn',
'orion_msc_i_kp': 'IRn',
'orion_msc_j_kp': 'IRn',
'BN_Mosaic_A_kp': 'Pare1839',
'BN_Mosaic_B_kp': 'Pare1839',
'BN_Mosaic_C_kp': 'Pare1839',
'BN_Mosaic_D_kp': 'Pare1839',
'BN_Mosaic_E_kp': 'ir1491',
'BN_Mosaic_F_kp': 'toller_4',
'BN_Mosaic_G_kp': 'Pare1839',
'BN_Mosaic_H_kp': 'Pare1839',
'BN_Mosaic_I_kp': 'ir1374',
'BN_Mosaic_J_kp': 'Pare1839',
'BN_Mosaic_K_kp': 'Pare1839',
}
# Initialize the Analysis object
Analysis.__init__(self,
epoch,
filt=filt,
rootDir=rootDir,
epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted,
cleanList=cleanList)
##########
# Setup the appropriate calibration stuff.
##########
self.calFile = '/g/lu/data/orion/source_list/' # old file: '/u/ghezgroup/data/orion/source_list/'
self.calFile += 'photo_calib.dat' # old file: 'photo_calib.dat'
self.calStars = self.mapFilter2CalStars[filt]
#self.calStars = None # use defaults in photo_calib file
# Choose the column based on the filter
self.calColumn = 3
# Set the coo star
self.cooStar = self.mapFilter2Coo[filt]
self.calCooStar = self.mapFilter2CalCoo[filt]
# Set the psf starlist
self.starlist = '/g/lu/code/idl/ucla_idl/'
self.starlist += 'orion/psfstars/psf_mosaic.dat'
self.labellist = '/g/lu/data/orion/source_list/label.dat'
self.orbitlist = None
#Set some default parameters
self.type = 'ao'
self.corrMain = 0.7
self.corrSub = 0.6
self.corrClean = 0.7
self.deblend = None
self.alignFlags = '-R 3 -v -p -a 0'
def __init__(self,
epoch,
field,
filt,
rootDir='/u/ghezgroup/data/gc/',
epochDirSuffix=None,
useDistorted=False,
cleanList='c.lis'):
"""
For Arches reduction:
epoch -- '06maylgs' for example
field -- 'f1', 'f2', etc. This sets the PSF star list to use.
filt -- 'kp', 'lp', or 'h'
"""
# Setup some Arches specific parameters
self.mapFilter2Cal = {'kp': 1, 'h': 2, 'lp': 3}
self.mapField2CooStar = {
'arch_f1': 'f1_psf0',
'arch_f2': 'f2_psf8',
'arch_f3': 'f3_psf0',
'arch_f4': 'f4_psf0',
'arch_f5': 'f5_psf1',
'arch_f6': 'f6_psf7'
}
self.mapField2CalStars = {
'arch_f1': [
'f1_psf0', 'f1_psf1', 'f1_psf2', 'f1_psf3', 'f1_psf4',
'f1_psf5', 'f1_psf6', 'f1_psf7', 'f1_psf9'
],
'arch_f2': [
'f2_psf0', 'f2_psf2', 'f2_psf3', 'f2_psf4', 'f2_psf6',
'f2_psf7', 'f2_psf8', 'f2_psf9', 'f2_psf10', 'f2_psf11',
'f2_psf12', 'f2_psf13'
],
'arch_f3': ['f3_psf0', 'f3_psf1', 'f3_psf5'],
'arch_f4': ['f4_psf0', 'f4_psf2'],
'arch_f5': [
'f5_psf0', 'f5_psf1', 'f5_psf2', 'f5_psf3', 'f5_psf4',
'f5_psf5', 'f5_psf12'
],
'arch_f6': ['f6_psf2', 'f6_psf3'],
}
# Initialize the Analysis object
Analysis.__init__(self,
epoch,
filt=field + '_' + filt,
rootDir=rootDir,
epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted,
cleanList=cleanList)
# Use the field to set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'arches/psfstars/%s_%s_psf_all.list' % \
(field, filt)
##########
# Setup the appropriate calibration stuff.
##########
# By default use the first 10 PSF stars.
self.calStars = self.mapField2CalStars[field]
# Choose the column based on the filter
self.calColumn = self.mapFilter2Cal[filt]
# Set the coo star
self.cooStar = self.mapField2CooStar[field]
self.calCooStar = self.cooStar
# Override some of the default parameters
# self.calFlags = '-f 1 -c 4 -R '
self.calFlags = '-f 1 -R '
self.calFile = '/u/ghezgroup/data/gc/source_list/photo_calib_arch.dat'
self.labellist = '/u/ghezgroup/data/gc/source_list/label_arch.dat'
self.orbitlist = None
def __init__(self, epoch, filt, rootDir='/g/lu/data/orion/2010oct/',
epochDirSuffix=None, useDistorted=False, cleanList='c.lis'):
"""
For reduction of deep wide mosaics:
epoch -- '06maylgs1' for example
filt -- 'dp_msc_C_kp', 'dp_msc_NE_kp', 'dp_msc_SE_kp', and so on...
"""
# Create dictionary which maps the PSF stars to the field
self.mapFilter2CalStars = {'orion_msc_a_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374'],
'orion_msc_b_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1366'],
'orion_msc_c_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1366'],
'orion_msc_d_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366', 'ir1486'],
'orion_msc_e_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_f_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_g_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_h_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_i_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'orion_msc_j_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1366'],
'BN_Mosaic_A_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1486', 'ir1519', 'toller_5', 'toller_6', 'toller_7', 'toller_8', 'toller_9', 'toller_10', 'CXOONC'],
'BN_Mosaic_B_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1486', 'ir1519', 'toller_5', 'toller_6', 'toller_7', 'toller_8', 'toller_9', 'toller_10', 'CXOONC'],
'BN_Mosaic_C_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1486', 'toller_6', 'toller_7', 'toller_8', 'toller_9', 'CXOONC', 'toller_10', 'toller_5', 'ir1519'],
'BN_Mosaic_D_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1486', 'toller_5', 'toller_6', 'toller_7', 'toller_8', 'toller_9', 'CXOONC', 'toller_10', 'toller_3'],
'BN_Mosaic_E_kp': ['Pare1839', 'ir1491', 'ir1486', 'toller_8', 'toller_9', 'toller_3', 'toller_2', 'toller_4', 'toller_11', 'toller_12', 'toller_13'],
'BN_Mosaic_F_kp': ['toller_4', 'toller_2', 'toller_3', 'toller_11', 'toller_12', 'toller_13'],
'BN_Mosaic_G_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1486', 'toller_5', 'toller_6', 'toller_7', 'toller_8', 'toller_9', 'toller_2', 'toller_3', 'CXOONC'],
'BN_Mosaic_H_kp': ['IRn', 'Pare1839', 'ir1374', 'ir1352', 'ir1486', 'toller_8', 'CXOONC', 'toller_10'],
'BN_Mosaic_I_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'CXOONC', 'toller_5', 'toller_6', 'toller_7', 'toller_9'],
'BN_Mosaic_J_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1519', 'ir1486', 'CXOONC', 'toller_5', 'toller_6', 'toller_7', 'toller_8', 'toller_9', 'toller_10'],
'BN_Mosaic_K_kp': ['IRn', 'Pare1839', 'ir1491', 'ir1374', 'ir1352', 'ir1519', 'ir1486', 'CXOONC', 'toller_5', 'toller_6', 'toller_7', 'toller_8', 'toller_9', 'toller_10'],
}
self.mapFilter2Coo = {'orion_msc_a_kp': 'IRn',
'orion_msc_b_kp': 'IRn',
'orion_msc_c_kp': 'IRn',
'orion_msc_d_kp': 'IRn',
'orion_msc_e_kp': 'IRn',
'orion_msc_f_kp': 'IRn',
'orion_msc_g_kp': 'IRn',
'orion_msc_h_kp': 'IRn',
'orion_msc_i_kp': 'IRn',
'orion_msc_j_kp': 'IRn',
'BN_Mosaic_A_kp': 'Pare1839',
'BN_Mosaic_B_kp': 'Pare1839',
'BN_Mosaic_C_kp': 'Pare1839',
'BN_Mosaic_D_kp': 'Pare1839',
'BN_Mosaic_E_kp': 'ir1491',
'BN_Mosaic_F_kp': 'toller_4',
'BN_Mosaic_G_kp': 'Pare1839',
'BN_Mosaic_H_kp': 'Pare1839',
'BN_Mosaic_I_kp': 'ir1374',
'BN_Mosaic_J_kp': 'Pare1839',
'BN_Mosaic_K_kp': 'Pare1839',
}
self.mapFilter2CalCoo = {'orion_msc_a_kp': 'IRn',
'orion_msc_b_kp': 'IRn',
'orion_msc_c_kp': 'ir1374',
'orion_msc_d_kp': 'IRn',
'orion_msc_e_kp': 'IRn',
'orion_msc_f_kp': 'IRn',
'orion_msc_g_kp': 'IRn',
'orion_msc_h_kp': 'IRn',
'orion_msc_i_kp': 'IRn',
'orion_msc_j_kp': 'IRn',
'BN_Mosaic_A_kp': 'Pare1839',
'BN_Mosaic_B_kp': 'Pare1839',
'BN_Mosaic_C_kp': 'Pare1839',
'BN_Mosaic_D_kp': 'Pare1839',
'BN_Mosaic_E_kp': 'ir1491',
'BN_Mosaic_F_kp': 'toller_4',
'BN_Mosaic_G_kp': 'Pare1839',
'BN_Mosaic_H_kp': 'Pare1839',
'BN_Mosaic_I_kp': 'ir1374',
'BN_Mosaic_J_kp': 'Pare1839',
'BN_Mosaic_K_kp': 'Pare1839',
}
# Initialize the Analysis object
Analysis.__init__(self, epoch, filt=filt,
rootDir=rootDir, epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted, cleanList=cleanList)
##########
# Setup the appropriate calibration stuff.
##########
self.calFile = '/g/lu/data/orion/source_list/' # old file: '/u/ghezgroup/data/orion/source_list/'
self.calFile += 'photo_calib.dat' # old file: 'photo_calib.dat'
self.calStars = self.mapFilter2CalStars[filt]
#self.calStars = None # use defaults in photo_calib file
# Choose the column based on the filter
self.calColumn = 3
# Set the coo star
self.cooStar = self.mapFilter2Coo[filt]
self.calCooStar = self.mapFilter2CalCoo[filt]
# Set the psf starlist
self.starlist = '/g/lu/code/idl/ucla_idl/'
self.starlist += 'orion/psfstars/psf_mosaic.dat'
self.labellist = '/g/lu/data/orion/source_list/label.dat'
self.orbitlist = None
#Set some default parameters
self.type = 'ao'
self.corrMain = 0.7
self.corrSub = 0.6
self.corrClean = 0.7
self.deblend = None
self.alignFlags = '-R 3 -v -p -a 0'
def __init__(self, epoch, filt, rootDir='/u/ghezgroup/data/gc/',
epochDirSuffix=None, useDistorted=False, cleanList='c.lis'):
"""
For reduction of deep wide mosaics:
epoch -- '06maylgs1' for example
filt -- 'dp_msc_C_kp', 'dp_msc_NE_kp', 'dp_msc_SE_kp', and so on...
"""
# Create dictionary which maps the PSF stars to the field
self.mapFilter2CalStars = {'dp_msc_C_kp': ['16C', '16NW', '16NE', '16CC', 'S2-16', '33N', 'S1-23', '33E', 'S2-22'],
'dp_msc_NE_kp': ['10EE', '10W', 'b100', 'S12-1', 'S11-6', 'irs17'],
'dp_msc_SE_kp': ['irs28', 'S12-2'],
'dp_msc_NW_kp': ['S8-3', 'S7-9', 'S10-2', 'S12-8', 'S12-4'],
'dp_msc_SW_kp': ['idSW2', 'S7-18'],
'dp_msc_E_kp': ['1SE', '1NE', 'S10-1', 'S5-183', 'irs28'],
'dp_msc_W_kp': ['S5-69', 'S7-18', 'irs2'],
'dp_msc_N_kp': ['irs7', 'S9-5', '15NE', 'S10-3', 'S11-6', 'S12-4'],
'dp_msc_S_kp': ['14NE', 'irs14SW', '12N'],
'dp_msc_C_SW_kp': ['irs2', 'S7-18', '12N', 'S1-23', '33N', 'irs14SW'],
'dp_msc_C_NE_kp': ['16C', '16NW', '16NE', '16CC', 'S2-22', '1NE', '1SE', '10W'],
'dp_msc_C_SE_kp': ['33E', '33N', 'S5-183', '14NE'],
'dp_msc_C_NW_kp': ['irs34W', 'S2-16', 'S5-69', 'S7-9', 'S8-3', '16NW', 'S1-23']
}
self.mapFilter2Coo = {'dp_msc_C_kp': 'irs16C',
'dp_msc_NE_kp': 'S11-6',
'dp_msc_SE_kp': 'S12-2',
'dp_msc_NW_kp': 'S8-3',
'dp_msc_SW_kp': 'S13-61',
'dp_msc_E_kp': 'S10-1',
'dp_msc_W_kp': 'S5-69',
'dp_msc_N_kp': 'S10-3',
'dp_msc_S_kp': 'irs14SW',
'dp_msc_C_SW_kp': 'irs2',
'dp_msc_C_NE_kp': 'irs16C',
'dp_msc_C_SE_kp': 'irs33E',
'dp_msc_C_NW_kp': 'irs34W'
}
self.mapFilter2CalCoo = {'dp_msc_C_kp': 'irs16C',
'dp_msc_NE_kp': 'S11-6',
'dp_msc_SE_kp': 'S12-2',
'dp_msc_NW_kp': 'S8-3',
'dp_msc_SW_kp': 'S13-61',
'dp_msc_E_kp': 'S10-1',
'dp_msc_W_kp': 'S5-69',
'dp_msc_N_kp': 'S10-3',
'dp_msc_S_kp': 'irs14SW',
'dp_msc_C_SW_kp': 'irs2',
'dp_msc_C_NE_kp': 'irs16C',
'dp_msc_C_SE_kp': 'irs33E',
'dp_msc_C_NW_kp': 'irs34W'
}
# Initialize the Analysis object
Analysis.__init__(self, epoch, filt=filt,
rootDir=rootDir, epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted, cleanList=cleanList)
##########
# Setup the appropriate calibration stuff.
##########
self.calFile = '/u/ghezgroup/data/gc/source_list/'
self.calFile += 'photo_calib_schoedel2010.dat'
#self.calStars = self.mapFilter2CalStars[filt]
self.calStars = None # use defaults in photo_calib file
# Choose the column based on the filter
self.calColumn = 2
# Set the coo star
self.cooStar = self.mapFilter2Coo[filt]
self.calCooStar = self.mapFilter2CalCoo[filt]
# Set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'gc/starfinder/psfstars/psf_mosaic.dat'
def __init__(self, epoch, filt, rootDir='/u/ghezgroup/data/gc/',
epochDirSuffix=None, useDistorted=False, cleanList='c.lis'):
# Create dictionary which maps the PSF stars to the field:
self.mapFilter2CalStars = {'h_lp': ['16C', '16NW', '16NE', '10W', '10EE', '1NE', '1SE', 'S2-22'],
'f_lp': ['10EE', '10W', 'S12-1', 'irs17', 'b100'],
'd_lp': ['irs28', '1SE', 'S13-1'],
'l_lp': ['irs7', 'S9-5', 'S10-3', 'S12-4', 'S10-2', '15NE', '15SW'],
'j_lp': ['33E', '33N', 'irs2', '14NE', 'S1-23'],
'e_lp': ['S12-1', 'S10-1', '1NE', '10EE', '1SE', 'S13-1'],
'k_lp': ['16C', '16NW', '16NE', '16CC', 'S2-16', 'S1-23', '33N'],
'r_lp': ['10W', '10EE', 'b100', 'S9-5'],
'i_lp': ['33E', '33N', '1SE', '14NE', 'S2-22'],
'c_lp': ['irc1', 'irc2'],
'b_lp': ['irb1', 'irb2', 'irb3'],
'a_lp': ['ira1', 'ira2', 'ira3'],
'p_lp': ['irp1', 'irp2', 'irp3'],
'q_lp': ['irq1', 'irq2'],
'r_lp': ['irr1', 'irr2'],
's_lp': ['irsf1', 'irsf2', 'irsf3'],
't_lp': ['irt1', 'irt2', 'irt3', 'irt4'],
'm_lp': ['irm1', 'irm2', 'im3'],
'n_lp': ['irn1'],
'tot_o_lp': ['iro1', 'iro2', 'iro3', 'iro4']
}
self.mapFilter2Coo = {'a_lp': ['ira_coo'],
'b_lp': ['irb_coo'],
'c_lp': ['irc_coo'],
'd_lp': ['irs28'],
'e_lp': ['S10-1'],
'f_lp': ['irs10EE'],
'g_lp': ['irs15NE'],
'h_lp': ['irs16C'],
'i_lp': ['irs14NE'],
'j_lp': ['S9-114'],
'k_lp': ['S5-69'],
'l_lp': ['S10-2'],
'm_lp': ['irm_coo'],
'n_lp': ['irn1'],
'o_lp': ['iro_coo'],
'p_lp': ['irp_coo'],
'q_lp': ['irq_coo'],
'r_lp': ['irr_coo'],
's_lp': ['irsf2'],
't_lp': ['irt_coo']
}
self.mapFilter2CalCoo = {'a_lp': ['ira_coo'],
'b_lp': ['irb_coo'],
'c_lp': ['irc_coo'],
'd_lp': ['irs28'],
'e_lp': ['S10-1'],
'f_lp': ['irs10EE'],
'g_lp': ['irs15NE'],
'h_lp': ['irs16C'],
'i_lp': ['irs14NE'],
'j_lp': ['S9-114'],
'k_lp': ['S5-69'],
'l_lp': ['S10-2'],
'm_lp': ['irm_coo'],
'n_lp': ['irn1'],
'o_lp': ['iro_coo'],
'p_lp': ['irp_coo'],
'q_lp': ['irq_coo'],
'r_lp': ['irr_coo'],
's_lp': ['irsf2'],
't_lp': ['irt_coo']
}
# Initialize the Analysis object
Analysis.__init__(self, epoch, filt=filt,
rootDir=rootDir, epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted, cleanList=cleanList, imgSuffix = '2')
##########
# Setup the appropriate calibration stuff.
##########
self.calStars = self.mapFilter2CalStars[filt]
# Choose the column based on the filter
self.calColumn = 3
# Set the coo star
self.cooStar = self.mapFilter2Coo[filt]
self.calCooStar = self.mapFilter2CalCoo[filt]
self.cooStar = self.mapFilter2Coo[filt]
self.calCooStar = self.mapFilter2CalCoo[filt]
# Set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'gc/starfinder/psfstars/psf_mosaic.dat'
def __init__(self, epoch, filt, rootDir='/u/ghezgroup/data/gc/',
epochDirSuffix=None, useDistorted=False, cleanList='c.lis'):
"""
For reduction of (shallow) maser mosaics:
epoch -- '06maylgs1' for example
filt -- 'msc_C_kp', 'msr_NE_kp', 'msr_SE_kp', and so on...
"""
# Create dictionary which maps the PSF stars to the field
self.mapFilter2CalStars = {'msr_C_kp': ['16C', '16NW', '16NE', '10W', '10EE', '1NE', '1SE', 'S2-22'],
'msr_NE_kp': ['10EE', '10W', 'S12-1', 'irs17', 'b100'],
'msr_SE_kp': ['irs28', '1SE', 'S13-1'],
'msr_NW_kp': ['irs7', 'S9-5', 'S10-3', 'S12-4', 'S10-2', '15NE', '15SW'],
'msr_SW_kp': ['33E', '33N', 'irs2', '14NE', 'S1-23'],
'msr_E_kp': ['S12-1', 'S10-1', '1NE', '10EE', '1SE', 'S13-1'],
'msr_W_kp': ['16C', '16NW', '16NE', '16CC', 'S2-16', 'S1-23', '33N'],
'msr_N_kp': ['10W', '10EE', 'b100', 'S9-5'],
'msr_S_kp': ['33E', '33N', '1SE', '14NE', 'S2-22']
}
self.mapFilter2Coo = {'msr_C_kp': ['irs16C'],
'msr_NE_kp': ['irs10EE'],
'msr_SE_kp': ['irs28'],
'msr_NW_kp': ['irs7'],
'msr_SW_kp': ['irs33N'],
'msr_E_kp': ['irs10EE'],
'msr_W_kp': ['irs16C'],
'msr_N_kp': ['S9-5'],
'msr_S_kp': ['irs33N']
}
self.mapFilter2CalCoo = {'msr_C_kp': ['16C'],
'msr_NE_kp': ['10EE'],
'msr_SE_kp': ['irs28'],
'msr_NW_kp': ['irs7'],
'msr_SW_kp': ['33N'],
'msr_E_kp': ['10EE'],
'msr_W_kp': ['16C'],
'msr_N_kp': ['S9-5'],
'msr_S_kp': ['33N']
}
# Initialize the Analysis object
Analysis.__init__(self, epoch, filt=filt,
rootDir=rootDir, epochDirSuffix=epochDirSuffix,
useDistorted=useDistorted, cleanList=cleanList)
##########
# Setup the appropriate calibration stuff.
##########
self.calStars = self.mapFilter2CalStars[filt]
# Choose the column based on the filter
self.calColumn = 2
# Set the coo star
self.cooStar = self.mapFilter2Coo[filt]
self.calCooStar = self.mapFilter2CalCoo[filt]
# Set the psf starlist
self.starlist = '/u/ghezgroup/code/idl/'
self.starlist += 'gc/starfinder/psfstars/psf_mosaic.dat'
