% CMB-S4 06 noise levels (DSR beamwidths, BK15 noise levels)
%
% SAT values from Ben post http://bicep.rc.fas.harvard.edu/CMB-S4/analysis_logbook/20190829_noise_params_DSR
% which are BK15 scaled to S4 bands by ratio of ideal NET values
% with no scaling of the number of detector years
% The hit pattern is implicitly the BK15 one - re-deploy the hits on sky to go to other
% patterns and boost the det-yrs using reldetyrs.dat file
%
% 1/f noise model parameters, fitted on the BK15 noise bandpowers 
% BC	BW	beam-fwhm	3x white-noise-level ell-knee 1/f-exponent for TT/EE/BB  	ellmin 	nside 
% GHz	GHz	arcmin	uK-arcmin
%
20	5.0	11.0	8.14	500	-4.3	5.52   200	-1.9	5.07   200	-1.5	30	512
30	9.0	72.8	6.73	150	-4.3	4.56	65	-1.9	4.20	75	-1.5	30	512
40	12.0	72.8	8.52	150	-4.3	5.78	65	-1.9	5.31	75	-1.5	30	512
85	20.4	25.5   10.27	150	-4.3	6.96	65	-1.9	6.40	75	-1.5	30	512
95	22.8	22.7	9.05	150	-4.3	6.14	65	-1.9	5.64	75	-1.5	30	512
145	31.9	25.5	9.31	230	-3.8	4.31	65	-3.0	4.21	60	-2.8	30	512
155	34.1	22.7	9.98	230	-3.8	4.61	65	-3.0	4.51	60	-2.8	30	512
220	48.4	13.0   74.81	220	-4.0   35.62	60	-3.1   34.59	60	-2.9	30	512
270	59.4	13.0  128.29	220	-4.0   61.08	60	-3.1   59.32	60	-2.9	30	512
%
% LAT values could come by same route from SPTpol N_ell's or similar
% Since those as not available use the numbers from DSR Table 2-2
% assuming these are for "Pole deep" hit pattern
  30     9.0     7.3     3.54   500     -4.3   5.00    200      -1.9    5.00   200      -1.5    30     2048
  40    12.0     5.5     3.18   500     -4.3   4.50    200      -1.9    4.50   200      -1.5    30     2048
  95    22.8     2.3     0.48   500     -4.3   0.68    200      -1.9    0.68   200      -1.5    30     2048
 145    31.9     1.5     0.68   500     -3.8   0.96    200      -3.0    0.96   200      -2.8    30     2048
 220    48.4     1.0     4.03   500     -4.0   5.70    200      -3.1    5.70   200      -2.9    30     2048
 270    59.4     0.8     6.93   500     -4.0   9.80    200      -3.1    9.80   200      -2.9    30     2048