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Merge pull request #504 from lsst/tickets/DM-42513
DM-42513: Scripts to add transmission_optics and transmission_filter data to obs_lsst_data for comCamSim
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python/lsst/obs/lsst/script/write_comCamSim_filter_files.py
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# This file is part of obs_lsst. | ||
# | ||
# Developed for the LSST Data Management System. | ||
# This product includes software developed by the LSST Project | ||
# (https://www.lsst.org). | ||
# See the COPYRIGHT file at the top-level directory of this distribution | ||
# for details of code ownership. | ||
# | ||
# This program is free software: you can redistribute it and/or modify | ||
# it under the terms of the GNU General Public License as published by | ||
# the Free Software Foundation, either version 3 of the License, or | ||
# (at your option) any later version. | ||
# | ||
# This program is distributed in the hope that it will be useful, | ||
# but WITHOUT ANY WARRANTY; without even the implied warranty of | ||
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the | ||
# GNU General Public License for more details. | ||
# | ||
# You should have received a copy of the GNU General Public License | ||
# along with this program. If not, see <https://www.gnu.org/licenses/>. | ||
import os | ||
import re | ||
import numpy as np | ||
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import astropy.units as u | ||
from astropy.table import QTable | ||
import dateutil.parser | ||
import galsim | ||
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import lsst.utils | ||
from lsst.meas.algorithms.simple_curve import DetectorCurve | ||
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# Write transmission_filter files for the g, r, i band used | ||
# by LSSTComCamSim. These are the baseline/filter_[gri].dat | ||
# files in the throughputs package. | ||
throughputs_dir = lsst.utils.getPackageDir("throughputs") | ||
filter_files = [ | ||
os.path.join(throughputs_dir, "baseline", _) | ||
for _ in ("filter_g.dat", "filter_r.dat", "filter_i.dat") | ||
] | ||
physical_filters = ("g_01", "r_03", "i_06") | ||
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for physical_filter, filter_file in zip(physical_filters, filter_files): | ||
throughput = np.genfromtxt(filter_file).transpose() | ||
# Use a GalSim.Bandpass object to truncate the curves at low | ||
# relative throughput and thin the number of wavelength points. | ||
bp = galsim.Bandpass( | ||
galsim.LookupTable(*throughput, interpolant="linear"), wave_type="nm" | ||
) | ||
bp = bp.truncate(relative_throughput=1e-4) | ||
bp = bp.thin() | ||
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# Package as a DetectorCurve object. | ||
optics_table = QTable( | ||
{ | ||
"wavelength": bp.wave_list * u.nanometer, | ||
"efficiency": bp(bp.wave_list) * 100.0 * u.percent, | ||
} | ||
) | ||
curve = DetectorCurve.fromTable(optics_table) | ||
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# Set metadata values. | ||
valid_start = "1970-01-01T00:00:00" | ||
optics_table.meta.update( | ||
{ | ||
"CALIBDATE": valid_start, | ||
"INSTRUME": "comCamSim", | ||
"OBSTYPE": "transmission_filter", | ||
"TYPE": "transmission_filter", | ||
"CALIBCLS": "lsst.ip.isr.IntermediateFilterTransmissionCurve", | ||
"SOURCE": "https://github.com/lsst/throughputs", | ||
"FILTER": physical_filter, | ||
"VERSION": 1.9, | ||
} | ||
) | ||
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optics_table.meta["CALIB_ID"] = f"calibDate={valid_start} filter={physical_filter}" | ||
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# Write output transmission_filter file. | ||
valid_date = dateutil.parser.parse(valid_start) | ||
datestr = "".join(re.split(r"[:-]", valid_date.isoformat())) | ||
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data_dir = lsst.utils.getPackageDir("obs_lsst_data") | ||
outfile = os.path.join( | ||
data_dir, "comCamSim", "transmission_filter", physical_filter, datestr + ".ecsv" | ||
) | ||
os.makedirs(os.path.dirname(outfile), exist_ok=True) | ||
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curve.writeText(outfile) |
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python/lsst/obs/lsst/script/write_comCamSim_optics_file.py
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# This file is part of obs_lsst. | ||
# | ||
# Developed for the LSST Data Management System. | ||
# This product includes software developed by the LSST Project | ||
# (https://www.lsst.org). | ||
# See the COPYRIGHT file at the top-level directory of this distribution | ||
# for details of code ownership. | ||
# | ||
# This program is free software: you can redistribute it and/or modify | ||
# it under the terms of the GNU General Public License as published by | ||
# the Free Software Foundation, either version 3 of the License, or | ||
# (at your option) any later version. | ||
# | ||
# This program is distributed in the hope that it will be useful, | ||
# but WITHOUT ANY WARRANTY; without even the implied warranty of | ||
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the | ||
# GNU General Public License for more details. | ||
# | ||
# You should have received a copy of the GNU General Public License | ||
# along with this program. If not, see <https://www.gnu.org/licenses/>. | ||
import os | ||
import re | ||
import numpy as np | ||
|
||
import astropy.units as u | ||
from astropy.table import QTable | ||
import dateutil.parser | ||
import galsim | ||
|
||
import lsst.utils | ||
from lsst.meas.algorithms.simple_curve import DetectorCurve | ||
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# Obtain the throughputs of the individual optical components from | ||
# the throughputs package. | ||
throughputs_dir = lsst.utils.getPackageDir("throughputs") | ||
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component_files = [ | ||
os.path.join(throughputs_dir, "baseline", _) | ||
for _ in ("m1.dat", "m2.dat", "m3.dat", "lens1.dat", "lens2.dat", "lens3.dat") | ||
] | ||
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# Combine, i.e., multiply, the component contributions to get the | ||
# total optical throughput. | ||
total = np.genfromtxt(component_files[0], names=["wl", "throughput"]) | ||
for component_file in component_files[1:]: | ||
component = np.genfromtxt(component_file, names=["wl", "throughput"]) | ||
total["throughput"] *= component["throughput"] | ||
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# Use a GalSim.Bandpass object to truncate the curves at low | ||
# relative throughput and thin the number of wavelength points. | ||
bp = galsim.Bandpass( | ||
galsim.LookupTable(total["wl"], total["throughput"], interpolant="linear"), | ||
wave_type="nm", | ||
) | ||
bp = bp.truncate(relative_throughput=1e-4) | ||
bp = bp.thin() | ||
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# Package as a DetectorCurve object. | ||
optics_table = QTable( | ||
{ | ||
"wavelength": bp.wave_list * u.nanometer, | ||
"efficiency": bp(bp.wave_list) * 100.0 * u.percent, | ||
} | ||
) | ||
curve = DetectorCurve.fromTable(optics_table) | ||
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# Set metadata values. | ||
valid_start = "1970-01-01T00:00:00" | ||
optics_table.meta.update( | ||
{ | ||
"CALIBDATE": valid_start, | ||
"INSTRUME": "comCamSim", | ||
"OBSTYPE": "transmission_optics", | ||
"TYPE": "transmission_optics", | ||
"CALIBCLS": "lsst.ip.isr.IntermediateOpticsTransmissionCurve", | ||
"SOURCE": "https://github.com/lsst/throughputs", | ||
"VERSION": 1.9, | ||
} | ||
) | ||
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optics_table.meta["CALIB_ID"] = f"calibDate={valid_start} filter=None" | ||
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# Write output transmission_optics file. | ||
valid_date = dateutil.parser.parse(valid_start) | ||
datestr = "".join(re.split(r"[:-]", valid_date.isoformat())) | ||
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data_dir = lsst.utils.getPackageDir("obs_lsst_data") | ||
outfile = os.path.join(data_dir, "comCamSim", "transmission_optics", datestr + ".ecsv") | ||
os.makedirs(os.path.dirname(outfile), exist_ok=True) | ||
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curve.writeText(outfile) |