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Color terms and Galactic extinction coefficients for DECam filters (including the Merian medium-band filters) #206

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12 changes: 12 additions & 0 deletions config/calibrate.py
Original file line number Diff line number Diff line change
Expand Up @@ -30,4 +30,16 @@
# See Slack: https://lsstc.slack.com/archives/C2B6X08LS/p1586468459084600
config.astrometry.wcsFitter.order = 4

# Photometric calibration: use color terms
config.photoCal.applyColorTerms = True
colors = config.photoCal.match.referenceSelection.colorLimits
# The following two color limits are adopted from obs_subaru for HSC SSP survey.
colors["g-r"] = ColorLimit(primary="g_flux", secondary="r_flux", minimum=0.0)
colors["r-i"] = ColorLimit(primary="r_flux", secondary="i_flux", maximum=0.5)
# The following magnitude limit is also adopted from obs_subaru for HSC SSP survey.
config.photoCal.match.referenceSelection.doMagLimit = True
config.photoCal.match.referenceSelection.magLimit.fluxField = "i_flux"
config.photoCal.match.referenceSelection.magLimit.maximum = 22.0
config.photoCal.colorterms.load(os.path.join(obsConfigDir, 'colorterms.py'))

config.measurement.load(os.path.join(obsConfigDir, "hsm.py"))
5 changes: 5 additions & 0 deletions config/colorAnalysis.py
Original file line number Diff line number Diff line change
@@ -0,0 +1,5 @@
import os.path

config.load(os.path.join(os.path.dirname(__file__), "extinctionCoeffs.py"))
from lsst.obs.decam.decamFilters import DECAM_FILTER_DEFINITIONS
config.physicalToBandFilterMap = DECAM_FILTER_DEFINITIONS.physical_to_band
51 changes: 51 additions & 0 deletions config/colorterms.py
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@@ -0,0 +1,51 @@
from lsst.pipe.tasks.colorterms import Colorterm, ColortermDict

# Average color terms for the DECam filters are calculated using the Pickles stellar spectra atlas.
# The following values are provided by Song Huang (Tsinghua University; [email protected])
# Color terms for u, Y, N964, and N419 bands are not available now.

# The values for DECam g, r, & z-band are calculated independently and are different with the values from: https://www.legacysurvey.org/dr9/description/
# A Jupyter notebook is available at https://github.com/MerianSurvey/caterpillar/blob/main/notebook/photocal/merian_filter_color_terms.ipynb
# to reproduce these values.

# In obs_subaru, colorterms.py is also used in:
# - config/jointcal.py
# - config/skyAnalysis.py
# - config/compareCoaddAnalysis.py
# - config/coaddAnalysis.py
# - config/visitAnalysis.py
# - config/fgcmBuildStarsTable.py and config/fgcmBuildStars.py
# These files are not available for obs_decam yet.

config.data = {
"decam*": ColortermDict(data={
'g': Colorterm(primary="g", secondary="g"),
'r': Colorterm(primary="r", secondary="r"),
'i': Colorterm(primary="i", secondary="i"),
'z': Colorterm(primary="z", secondary="z"),
}),
"sdss*": ColortermDict(data={
'g': Colorterm(primary="g", secondary="r", c0=-0.008015, c1=-0.089869, c2=-0.018398), # For -1.0 < g-r < 1.8
'r': Colorterm(primary="r", secondary="i", c0=-0.0077434, c1=-0.202615, c2=0.016042), # For -1.0 < r-i < 2.2
'i': Colorterm(primary="i", secondary="z", c0=0.00018887, c1=-0.2748281, c2=-0.029417), # For -1.0 < i-z < 1.2
'z': Colorterm(primary="z", secondary="i", c0=-0.0059858, c1=0.1131192, c2=0.0156471), # For -1.0 < z-i < 0.5
'N708': Colorterm(primary="r", secondary="i", c0=-0.01428724, c1=-0.71755905, c2=0.08959316), # For -1.0 < r-i < 2.0
'N540': Colorterm(primary="g", secondary="r", c0=-0.03359776, c1=-0.57665033, c2=-0.01510509), # For -1.0 < g-r < 1.5
}),
"hsc*": ColortermDict(data={
'g': Colorterm(primary="g", secondary="r", c0=0.0000509, c1=-0.0152487, c2=-0.0029937), # For -1.0 < g-r < 1.4
'r': Colorterm(primary="r", secondary="i", c0=-0.0078995, c1=-0.1695323, c2=0.0251978), # For -1.0 < r-i < 2.2
'i': Colorterm(primary="i", secondary="z", c0=0.0010196, c1=-0.1314031, c2=0.0054605), # For -1.0 < i-z < 1.0
'z': Colorterm(primary="z", secondary="y", c0=-0.0013244, c1=-0.2846684, c2=-0.1229817), # For -1.0 < z-y < 0.5
'N708': Colorterm(primary="r", secondary="i", c0=-0.01978413, c1=-0.64368838, c2=0.09132738), # For -1.0 < r-i < 2.0
'N540': Colorterm(primary="g", secondary="r", c0=-0.03015158, c1=-0.53715834, c2=-0.00202415), # For -1.0 < g-r < 1.5
}),
"ps1*": ColortermDict(data={
'g': Colorterm(primary="g", secondary="r", c0=0.006388, c1=0.045875, c2=-0.004484), # For -1.0 < g-r < 1.2
'r': Colorterm(primary="r", secondary="i", c0=-0.006775, c1=-0.187304, c2=0.018928), # For -1.0 < r-i < 2.2
'i': Colorterm(primary="i", secondary="z", c0=0.0012204, c1=-0.282956, c2=-0.011321), # For -1.0 < i-z < 1.4
'z': Colorterm(primary="z", secondary="y", c0=-0.0087868, c1=-0.5204795, c2=-0.057955), # For -1.0 < z-y < 1.0
'N708': Colorterm(primary="r", secondary="i", c0=-0.01508987, c1=-0.69377675, c2=0.09079348), # For -1.0 < r-i < 2.0
'N540': Colorterm(primary="g", secondary="r", c0=-0.02635164, c1=-0.50968428, c2=-0.00958104), # For -1.0 < g-r < 1.5
}),
}
15 changes: 15 additions & 0 deletions config/extinctionCoeffs.py
Original file line number Diff line number Diff line change
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# Extinction coefficients for DECam filters for conversion from E(B-V) to extinction, A_filter.
# Numbers provided by Song Huang (NAOJ).
#
# Band, A_filter/E(B-V)
# Values for N964 and N149 filters are not available at this point.
config.extinctionCoeffs = {
"u": 3.994,
"g": 3.212,
"r": 2.164,
"i": 1.591,
"z": 1.211,
"y": 1.063,
"N708": 1.847,
"N540": 2.753
}