# Units:
#  "lambda" is in Angstroms
#  "pass" is the contribution to the detector signal per photon
#         entering the atmosphere of Earth
#
# Bandpass Name(s): I
#
# Instrument: Hypothetical system developed to match known "standards"
#             of Johnson/Cousins to spectrophotometry
# 
# Determined by: M. S. Bessell
#
# Date of determination: 1990
#
# Meaning of/Reason for default column: Only available
#
# Notes:
#
# These filter curves define the "official" Johnson/Cousins BVRI
# system, as far # as I am concerned. One must take care to make sure
# that you really want these filters; ie. that the observations have
# been converted into this system. Otherwise, you will have to use
# custom filter curves (which may not be a bad idea).
# 
# Details of how/why this system is defined can be found in:
#
# Bessell, M.S. 1990, PASP, 102, 1181
#
# Read it; it will give you a good insight into how complex this 
# whole business really is.
#
# Michael Blanton
# 2002-08-19
#

typedef struct {
  double lambda;
  double pass;
} KFILTER;

KFILTER 7000. 0
KFILTER 7100. 0.0169014084507042
KFILTER 7200. 0.161111111111111
KFILTER 7300. 0.38013698630137
KFILTER 7400. 0.530405405405405
KFILTER 7500. 0.606666666666667
KFILTER 7600. 0.634868421052632
KFILTER 7700. 0.63961038961039
KFILTER 7800. 0.634615384615385
KFILTER 7900. 0.629746835443038
KFILTER 8000. 0.625
KFILTER 8100. 0.617283950617284
KFILTER 8200. 0.603658536585366
KFILTER 8300. 0.590361445783133
KFILTER 8400. 0.56547619047619
KFILTER 8500. 0.535294117647059
KFILTER 8600. 0.5
KFILTER 8700. 0.431034482758621
KFILTER 8800. 0.318181818181818
KFILTER 8900. 0.185393258426966
KFILTER 9000. 0.0833333333333333
KFILTER 9100. 0.0164835164835165
KFILTER 9200. 0