Optimal Telescope Selection

Choose to leave out:
NANOGrav

PPTA

EPTA
 Observation Time:
# of Obs per year:
Amplitude of background:
IPTA
PPTA
EPTA
NANOGrav

Selected Pulsars:

Calculate RMS:
PulsarRMS (ns)



Array:     

False Alarm Probability:    

Detection Probability:    


(1 - False Dissmissal)

Cadence

Background Spectral Index

Max Amplitude

Statistic

 Minimum Detectable Amplitude
(for a SMBH Binary Background)
year
 year
 year
Alpha
         
Beta
           
Gamma
           
Delta
         
       Correlation vs Angle Between Pulsar Plot