diff --git a/python/lsst/obs/lsst/script/rewrite_latiss_optics_file.py b/python/lsst/obs/lsst/script/rewrite_latiss_optics_file.py
new file mode 100644
index 000000000..b0c36cb1a
--- /dev/null
+++ b/python/lsst/obs/lsst/script/rewrite_latiss_optics_file.py
@@ -0,0 +1,82 @@
+# 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 dateutil.parser
+
+import numpy as np
+import astropy.units as u
+from astropy.table import Table, QTable
+
+import lsst.utils
+from lsst.meas.algorithms.simple_curve import DetectorCurve
+
+
+data_dir = lsst.utils.getPackageDir("obs_lsst_data")
+subaru_file = "subaru_m1_r_20200219.txt"
+valid_start = "1970-01-01T00:00:00"
+
+filename = os.path.join(data_dir, "latiss", "transmission_optics", subaru_file)
+
+subaru_data = Table.read(filename, format="ascii")
+
+wavelength = subaru_data["col1"]
+ref = np.mean(
+    np.array(subaru_data[["col2", "col3", "col4", "col5", "col6"]]).view("f8").reshape((len(subaru_data), 5)),
+    axis=1,
+)
+
+# Make sure it's sorted by wavelength.
+st = np.argsort(wavelength)
+
+optics_table = QTable(
+    {
+        "wavelength": np.array(wavelength[st], dtype=np.float64)*u.nanometer,
+        "efficiency": ref[st]*u.percent,
+    }
+)
+
+# Adjust the overall normalization to match AuxTel scans.
+optics_table["efficiency"] += 3.5*u.percent
+
+curve = DetectorCurve.fromTable(optics_table)
+
+valid_date = dateutil.parser.parse(valid_start)
+datestr = ''.join(re.split(r'[:-]', valid_date.isoformat()))
+
+outfile = os.path.join(data_dir, "latiss", "transmission_optics", datestr + ".ecsv")
+
+optics_table.meta.update(
+    {
+        "CALIBDATE": valid_start,
+        "INSTRUME": "LATISS",
+        "OBSTYPE": "transmission_optics",
+        "TYPE": "transmission_optics",
+        "CALIBCLS": "lsst.ip.isr.IntermediateOpticsTransmissionCurve",
+        "SOURCE": subaru_file,
+    }
+)
+
+optics_table.meta["CALIB_ID"] = (
+    f"calibDate={valid_start} filter=None"
+)
+
+curve.writeText(outfile)
diff --git a/python/lsst/obs/lsst/script/rewrite_latiss_qe_file.py b/python/lsst/obs/lsst/script/rewrite_latiss_qe_file.py
new file mode 100644
index 000000000..ff09a11a2
--- /dev/null
+++ b/python/lsst/obs/lsst/script/rewrite_latiss_qe_file.py
@@ -0,0 +1,118 @@
+# 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 astropy.units as u
+from astropy.io import fits
+from astropy.table import QTable
+import re
+import os
+import dateutil.parser
+import numpy
+
+import lsst.utils
+from lsst.meas.algorithms.simple_curve import AmpCurve
+
+amp_name_map = {'AMP01': 'C10', 'AMP02': 'C11', 'AMP03': 'C12', 'AMP04': 'C13', 'AMP05': 'C14',
+                'AMP06': 'C15', 'AMP07': 'C16', 'AMP08': 'C17', 'AMP09': 'C07', 'AMP10': 'C06',
+                'AMP11': 'C05', 'AMP12': 'C04', 'AMP13': 'C03', 'AMP14': 'C02', 'AMP15': 'C01',
+                'AMP16': 'C00'}
+
+
+def convert_qe_curve(filename):
+    """Convert a single QE curve from its native FITS format to an
+    an `astropy.table.QTable` representation.
+
+    Parameters
+    ----------
+    filename : `str`
+        Full path, including filename for the file to be converted.
+
+    Returns
+    -------
+    table : `astropy.table.QTable`
+        A QTable object containing the columns that describe this
+        QE curve.
+
+    Notes
+    -----
+    This function is specific to how the ts8 data are formatted
+    with a curve per amp.  If ther are other formats, a different
+    converter will be necessary.
+    """
+    with fits.open(filename) as hdu_list:
+        # qe data is in first extension
+        data = hdu_list[1].data
+    wlength = []
+    eff = dict()
+    for row in data:
+        wlength.append(row['WAVELENGTH'])
+        for i in range(16):  # There are 16 amps
+            col_name = f'AMP{i+1:02d}'
+            eff.setdefault(amp_name_map[col_name], []).append(row[col_name])
+    out_data = {'amp_name': [], 'wavelength': [], 'efficiency': []}
+    for k in eff:
+        amp_names = [k]*len(wlength)
+        out_data['amp_name'] += amp_names
+        out_data['wavelength'] += wlength
+        out_data['efficiency'] += eff[k]
+
+    out_data['amp_name'] = numpy.array(out_data['amp_name'])
+    out_data['wavelength'] = numpy.array(out_data['wavelength'])*u.nanometer
+    out_data['efficiency'] = numpy.array(out_data['efficiency'])*u.percent
+
+    return QTable(out_data)
+
+
+data_dir = lsst.utils.getPackageDir("obs_lsst_data")
+raft_name = "rxx"
+detector_name = "s00"
+raft_detector = raft_name + "_" + detector_name
+detector_id = 0
+fits_file = "ITL-3800C-068_QE.fits"
+valid_start = "1970-01-01T00:00:00"
+
+filename = os.path.join(data_dir, "latiss", "transmission_sensor", raft_detector, fits_file)
+
+curve_table = convert_qe_curve(filename)
+curve = AmpCurve.fromTable(curve_table)
+
+valid_date = dateutil.parser.parse(valid_start)
+datestr = ''.join(re.split(r'[:-]', valid_date.isoformat()))
+
+outfile = os.path.join(data_dir, "latiss", "transmission_sensor", raft_detector, datestr + ".ecsv")
+
+curve_table.meta.update(
+    {
+        "CALIBDATE": valid_start,
+        "INSTRUME": "LATISS",
+        "OBSTYPE": "transmission_sensor",
+        "TYPE": "transmission_sensor",
+        "DETECTOR": detector_id,
+        "CALIBCLS": "lsst.ip.isr.IntermediateSensorTransmissionCurve",
+        "SOURCE": fits_file,
+    }
+)
+
+curve_table.meta["CALIB_ID"] = (
+    f"raftName={raft_name} detectorName={detector_name} "
+    f"detector={detector_id} calibDate={valid_start} "
+    f"ccd={detector_id} ccdnum={detector_id} filter=None")
+
+curve.writeText(outfile)