Reconstructing the cosmic history of the most common MBHs populating galaxies today [1.0 yr]

FoM

Science investigation and Observational requirement: SI2.2 OR2.2a from Science requirement document.

Detection of MBHBs with source-frame mass in the range \(10^4-10^6\) M\(_\odot\) and formation redshift in the range \(z = 6-9\) with SNR\(>50\)

- GREAT 95.02555825438212 [50 75 90] : SO2 Reconstructing the cosmic history of the most common MBHs populating galaxies today

Assuming detection threshold 50. Detectability is OK if probability of detection > %75

Summary

MBHB with waveform IMRPhenomHM of

  • mass in 1.000000e+04-1.000000e+06 solar mass (log uniform)
  • mass ratio in [1, 10] (log uniform),
  • redshift in [6, 9] (uniform in comoving volume)
  • t0 in [0.10 - 0.95] (uniform)
  • chi in [0.00 - 0.99] (uniform))

Conducting monte-carlo over 10000 trials, randomizing spins, sky position and orientation

Assuming SNR threshold for detection: 50.0

Detailed results

waveform_params

'''

  • minf : 2e-05
  • maxf : 1
  • fend : None
  • tmin : 0.0
  • tmax : None
  • phiref : 0.0
  • fref_for_phiref : 0.0
  • toffset : 0.0
  • TDI : TDI2AET
  • acc : 0.0001
  • order_fresnel_stencil : 0
  • approximant : IMRPhenomHM
  • responseapprox : full
  • frozenLISA : False
  • TDIrescaled : False
  • LISAconst : {'OrbitOmega': 1.9909865927683783e-07, 'OrbitPhi0': 0.0, 'Orbitt0': 0.0, 'OrbitR': 149597870700.0, 'OrbitL': 2500000000.0}
  • LISAnoise : [[ 2.00000000e-05 3.26116899e-45 3.26116899e-45 -2.35000529e-51] [ 2.10000000e-05 3.04638010e-45 3.04638010e-45 -2.59086519e-51] [ 2.20000000e-05 2.86794944e-45 2.86794944e-45 -2.84347125e-51] ... [ 9.99998000e-01 1.12081104e-36 1.12081104e-36 2.92351422e-36] [ 9.99999000e-01 1.12081125e-36 1.12081125e-36 2.92372017e-36] [ 1.00000000e+00 1.12081141e-36 1.12081141e-36 2.92392603e-36]] '''

Input parameters


- log : log/SO2_detectability.c3.log
- config : config.yml
- subconfig : 
- duration : 1.0 yr
- duty_cycle : 1
- armlength : 2500000000.0 m
- noise : CBE_1yr_6yr_tdi2/noise_background_1_yr.npy
- show : False
- fast : 0
- tdi2 : 1
- freqs : [2e-05, 1]
- force_duration : 1_yr
- report : CBE_1yr_6yr_tdi2/report_SO2a_detectability.c3.md
- random_seed : 2137
- mass_range : [10000.0, 1000000.0]
- z_range : [6, 9]
- mass_ratio_range : [1, 10]
- snr_thresh : 50
- fom_range : [50, 75, 90]
- fom_title : Reconstructing the cosmic history of the most common MBHs populating galaxies today
- fom_or : ['SI2.2 OR2.2a']
- fom_objective : Detectability/PE for MBHB
- fom_config : SO2/detectability.c3.yml
- nproc : 24
- fom_obj : Detection of MBHBs with source-frame mass in the range $10^4-10^6$ M$_\odot$ and formation redshift in the range $z = 6-9$ with SNR$>50$

Download

SNR data c3