LSSTApplications  17.0+124,17.0+14,17.0+73,18.0.0+37,18.0.0+80,18.0.0-4-g68ffd23+4,18.1.0-1-g0001055+12,18.1.0-1-g03d53ef+5,18.1.0-1-g1349e88+55,18.1.0-1-g2505f39+44,18.1.0-1-g5315e5e+4,18.1.0-1-g5e4b7ea+14,18.1.0-1-g7e8fceb+4,18.1.0-1-g85f8cd4+48,18.1.0-1-g8ff0b9f+4,18.1.0-1-ga2c679d+1,18.1.0-1-gd55f500+35,18.1.0-10-gb58edde+2,18.1.0-11-g0997b02+4,18.1.0-13-gfe4edf0b+12,18.1.0-14-g259bd21+21,18.1.0-19-gdb69f3f+2,18.1.0-2-g5f9922c+24,18.1.0-2-gd3b74e5+11,18.1.0-2-gfbf3545+32,18.1.0-26-g728bddb4+5,18.1.0-27-g6ff7ca9+2,18.1.0-3-g52aa583+25,18.1.0-3-g8ea57af+9,18.1.0-3-gb69f684+42,18.1.0-3-gfcaddf3+6,18.1.0-32-gd8786685a,18.1.0-4-gf3f9b77+6,18.1.0-5-g1dd662b+2,18.1.0-5-g6dbcb01+41,18.1.0-6-gae77429+3,18.1.0-7-g9d75d83+9,18.1.0-7-gae09a6d+30,18.1.0-9-gc381ef5+4,w.2019.45
LSSTDataManagementBasePackage
findCosmicRaysConfig.py
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1 #
2 # LSST Data Management System
3 #
4 # Copyright 2008-2017 AURA/LSST.
5 #
6 # This product includes software developed by the
7 # LSST Project (http://www.lsst.org/).
8 #
9 # This program is free software: you can redistribute it and/or modify
10 # it under the terms of the GNU General Public License as published by
11 # the Free Software Foundation, either version 3 of the License, or
12 # (at your option) any later version.
13 #
14 # This program is distributed in the hope that it will be useful,
15 # but WITHOUT ANY WARRANTY; without even the implied warranty of
16 # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
17 # GNU General Public License for more details.
18 #
19 # You should have received a copy of the LSST License Statement and
20 # the GNU General Public License along with this program. If not,
21 # see <https://www.lsstcorp.org/LegalNotices/>.
22 #
23 import lsst.pex.config as pexConfig
24 from .subtractBackground import SubtractBackgroundTask
25 
26 
27 class FindCosmicRaysConfig(pexConfig.Config):
28  """Config for the findCosmicRays function
29  """
30  nCrPixelMax = pexConfig.Field(
31  dtype=int,
32  doc="maximum number of contaminated pixels",
33  default=10000,
34  )
35  minSigma = pexConfig.Field(
36  dtype=float,
37  doc="CRs must be > this many sky-sig above sky",
38  default=6.0,
39  )
40  min_DN = pexConfig.Field(
41  dtype=float,
42  doc="CRs must have > this many DN (== electrons/gain) in initial detection",
43  default=150.0,
44  )
45  cond3_fac = pexConfig.Field(
46  dtype=float,
47  doc="used in condition 3 for CR; see CR.cc code",
48  default=2.5,
49  )
50  cond3_fac2 = pexConfig.Field(
51  dtype=float,
52  doc="used in condition 3 for CR; see CR.cc code",
53  default=0.6,
54  )
55  niteration = pexConfig.Field(
56  dtype=int,
57  doc="number of times to look for contaminated pixels near known CR pixels",
58  default=3,
59  )
60  keepCRs = pexConfig.Field(
61  dtype=bool,
62  doc="Don't interpolate over CR pixels",
63  default=False,
64  )
65  background = pexConfig.ConfigurableField(
66  target=SubtractBackgroundTask,
67  doc="Background estimation configuration"
68  )
69 
70  def setDefaults(self):
71  self.background.useApprox = False
72  self.background.binSize = 100000
73  self.background.statisticsProperty = "MEDIAN"
74  self.background.undersampleStyle = "REDUCE_INTERP_ORDER"
75  self.background.algorithm = "AKIMA_SPLINE"