Difference between revisions of "Expected Survey Performance for Science Forecasting"

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(Observation Definition)
(Observation Definition)
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=== Observation Definition ===
 
=== Observation Definition ===
  
'''Delensing LAT'''
 
  
'''Wide-Area LAT'''
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'''Deep and Wide Field (Hi-res)'''
  
 
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'''Hi-res Ultra-deep Field '''
  
'''Pole SAT'''
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'''Lo-Res Ultra-Deep Field'''
 
 
'''Atacama SAT'''
 
  
  

Revision as of 14:23, 27 May 2019

The most up-to-date expected survey performances (previously called "experiment definitions"), and all the historical ones used for iterating, for both large-area survey and small-area survey, can be found at Survey Performance Expectations.

Expected Survey Performances (a result of instrument performance and observations) below are the converged result at each epoch (or will be once someone fills them in).


Reference Design

Instrument Definition

LAT

SAT

Observation Definition

Deep and Wide Field (Hi-res)

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) 9.5 11.5 1.5 2.1 7.9 13.8
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) 13.4 16.3 2.2 2.9 11.2 19.6
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

Hi-res Ultra-deep Field

Lo-Res Ultra-Deep Field



CDT Design

Instrument Definition

LAT

SAT

Observation Definition

Delensing LAT

Wide-Area LAT

Pole SAT

Atacama SAT