Difference between revisions of "WAFTT results part 3"

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Columns are no elevation penalty, with elevation penalty, and high cadence.
 
Columns are no elevation penalty, with elevation penalty, and high cadence.
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 +
These depth maps are for 254 detectors (127 pairs) taking data for one year. To arrive at the noise properties for the seven year survey, the noise levels obtained from these maps are rescaled by the number of detectors in the different frequency bands, taking into account a yield of 80% and correlation between detectors taken from [https://docs.google.com/spreadsheets/d/17KtDIc7pHTdL2F_22RZHve7l0vf-IY_YwMDVXQoEdnE/edit#gid=0 here]. In addition, they are scaled from a single year to seven years, assuming an efficiency of 23%, consistent with the assumptions that enter the noise calculator.
  
 
===Noise characteristics for minimum elevation of 50 degrees===
 
===Noise characteristics for minimum elevation of 50 degrees===

Revision as of 14:13, 6 June 2019

Summary

In this posting we study the effects of different scan strategies in the presence of atmospheric effects on the forecasts of Neff.

Depth maps

Total depth 095GHz.png

Rows are minimum observing elevations of 30, 40 and 50 degrees.

Columns are no elevation penalty, with elevation penalty, and high cadence.

These depth maps are for 254 detectors (127 pairs) taking data for one year. To arrive at the noise properties for the seven year survey, the noise levels obtained from these maps are rescaled by the number of detectors in the different frequency bands, taking into account a yield of 80% and correlation between detectors taken from here. In addition, they are scaled from a single year to seven years, assuming an efficiency of 23%, consistent with the assumptions that enter the noise calculator.

Noise characteristics for minimum elevation of 50 degrees

No elevation penalty

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 56.8 52.0 45.2 38.9
Effective sky fraction for noise (in %) 51.6 47.1 40.8 34.8
Effective sky fraction for signal (in %) 47.3 43.0 37.2 31.6


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 17.9 9.8 1.6 1.6 5.5 13.0
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 25.2 13.8 2.3 2.2 7.8 18.5
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1

With elevation penalty

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 56.8 52.0 45.2 38.8
Effective sky fraction for noise (in %) 51.1 46.6 40.4 34.3
Effective sky fraction for signal (in %) 45.9 41.7 36.0 30.6


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 17.4 9.6 1.6 1.5 5.4 12.8
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 24.8 13.5 2.3 2.2 7.6 18.1
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1

High cadence survey - 2 elevations

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 57.9 52.7 45.6 39.4
Effective sky fraction for noise (in %) 47.3 43.1 37.1 31.7
Effective sky fraction for signal (in %) 38.2 34.8 30.0 25.3


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 17.2 9.5 1.6 1.5 5.3 12.6
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 24.3 13.4 2.3 2.2 7.4 17.8
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1

High cadence survey - 11 elevations

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 59.7 54.4 47.2 40.8
Effective sky fraction for noise (in %) 53.9 49.2 42.5 36.6
Effective sky fraction for signal (in %) 48.3 44.1 37.9 32.5


Frequency (GHz) 30 40 90 150 220 270
white noise level TT (uK-arcmin) 18.8 10.5 1.8 1.7 5.9 13.9
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 26.4 14.8 2.4 2.3 8.2 19.7
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1

Noise characteristics for minimum elevation of 40 degrees

No elevation penalty

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 68.2 62.5 55.1 48.1
Effective sky fraction for noise (in %) 63.5 58.3 51.2 44.5
Effective sky fraction for signal (in %) 59.2 54.3 47.5 41.1


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 20.0 11.2 1.9 1.8 6.3 15.0
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 28.3 15.9 2.7 2.5 8.8 21.3
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.01 1.03 1.02 1.02 1.03 1.03

With elevation penalty

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 68.2 62.6 55.2 4812
Effective sky fraction for noise (in %) 61.3 56.2 49.3 42.7
Effective sky fraction for signal (in %) 54.9 50.2 43.8 37.7


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 19.3 10.6 1.8 1.7 6.0 14.0
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 27.3 14.9 2.6 2.3 8.4 19.8
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.00 1.01 1.01 1.01 1.01 1.01

High cadence survey - 2 elevations

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 67.6 61.4 53.9 46.8
Effective sky fraction for noise (in %) 58.6 53.3 46.4 39.4
Effective sky fraction for signal (in %) 50.0 45.5 39.4 33.8


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 19.5 11.1 1.9 1.8 6.2 15.0
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 27.5 15.8 2.6 2.4 8.8 21.1
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.03 1.06 1.04 1.04 1.06 1.07

High cadence survey - 11 elevations

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 69.8 63.6 56.0 48.7
Effective sky fraction for noise (in %) 62.6 56.9 49.7 43.1
Effective sky fraction for signal (in %) 55.6 50.6 43.9 37.9


Frequency (GHz) 30 40 90 150 220 270
white noise level TT (uK-arcmin) 20.7 11.9 2.0 1.9 6.7 16.1
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 29.4 16.8 2.9 2.6 9.4 22.7
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.03 1.06 1.05 1.04 1.06 1.07

Noise characteristics for minimum elevation of 30 degrees

No elevation penalty

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 75.8 69.3 61.6 53.9
Effective sky fraction for noise (in %) 70.9 64.8 57.3 50.1
Effective sky fraction for signal (in %) 66.2 60.6 53.3 46.5


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 21.8 12.4 2.0 2.0 6.9 16.7
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 30.8 17.6 2.9 2.8 9.8 23.6
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.04 1.08 1.06 1.06 1.07 1.09

With elevation penalty

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 75.8 69.3 61.6 53.9
Effective sky fraction for noise (in %) 66.1 60.5 53.3 46.4
Effective sky fraction for signal (in %) 57.6 52.7 46.1 39.8


Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 20.2 11.0 1.9 1.8 6.2 14.7
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 28.7 15.7 2.7 2.5 8.8 20.9
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.00 1.02 1.01 1.01 1.02 1.02

High cadence - 2 elevations

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 75.3 68.3 60.3 52.6
Effective sky fraction for noise (in %) 65.5 59.5 52.2 45.5
Effective sky fraction for signal (in %) 54.1 49.2 42.7 37.4
Frequency (GHz) 30 40 95 145 220 270
white noise level TT (uK-arcmin) 22.0 13.0 2.2 2.0 7.2 17.5
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 31.2 18.4 3.0 2.8 10.2 24.8
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.08 1.17 1.13 1.12 1.15 1.18

High cadence - 11 elevations

Galactic cut (in %) 0 10 20 30
Sky fraction (in %) 77.8 70.7 62.6 54.7
Effective sky fraction for noise (in %) 67.0 60.9 53.5 46.6
Effective sky fraction for signal (in %) 57.4 52.3 45.7 39.6


Frequency (GHz) 30 40 90 150 220 270
white noise level TT (uK-arcmin) 22.7 13.6 2.2 2.1 7.5 18.5
ell knee TT 433 395 1315 4651 4511 4525
1/f exponent TT (uK-arcmin) -3.5 -3.4 -3.1 -2.3 -3.4 -3.4
white noise level E/B (uK-arcmin) 32.1 19.3 3.1 2.9 10.6 26.1
ell knee E/B 467 467 467 467 467 467
1/f exponent E/B (uK-arcmin) -1.1 -1.1 -1.1 -1.1 -1.1 -1.1
Penalty (relative to f_sky scaling) 1.08 1.17 1.14 1.12 1.16 1.19

Results

Neff WAFTT v3 hc11.png