imrphenomhm_pe_study
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imrphenomhm_pe_study [2017/09/15 11:47] – chinmay.kalaghatgi@LIGO.ORG | imrphenomhm_pe_study [2017/09/18 14:11] (current) – [PE Runs] chinmay.kalaghatgi@LIGO.ORG | ||
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* The total response of a detector network (2 detector) is taken to be : sqrt( F< | * The total response of a detector network (2 detector) is taken to be : sqrt( F< | ||
- | * The response function depends on the ra, dec values of the sky-position along with the polarisation of the waveform and gps trigger time. So, we fix the polarisation to 1.75 radians (~ 100 deg) and the gps time to 1187128000. Constraining the values of ra, dec between (0, 2 pi) and (-pi/2, pi/2) respectively, | + | * The response function depends on the ra, dec values of the sky-position along with the polarisation of the waveform and gps trigger time. So, we fix the polarisation to 1.75 radians (~ 100 deg) and the gps time to 1187128000. Constraining the values of ra, dec between (0, 2 pi) and (-pi/2, pi/2) respectively, |
* {{: | * {{: | ||
| | ||
* {{: | * {{: | ||
+ | |||
+ | === Creating frame files === | ||
+ | |||
+ | * First, create a h5 file from the psi4 data for the different simulations. The script to create the h5 file is at : __/ | ||
+ | * As of 18/09/2017; I have created h5 files for q1, q2, q4, q8 and q18 non-spinning NR waveforms. q1 and q2 are Gerogia Tech waveforms while q4, q8 and q18 are BAM. | ||
+ | * I wanted to keep the f_low (as calculated from the NR waveform) of the waveform for all the systems to be the same, so I adjust the mass of the injection to adjust the f_low ~ 20Hz for all runs. | ||
+ | * Created HL and HVL (inclination series) frame files for the q4 and q8 non-spinning systems. To ensure f_low is same, q4 is injected at 80 Msun and q8 at 115 Msun. | ||
+ | * The two detector network injection (H-L) frames can be found at : __/ | ||
+ | * The three detector network injection (H-L-V) frames can be found at: __/ | ||
+ | |||
+ | |||
+ | === PE Runs === | ||
+ | |||
+ | * In some previous runs, we had noticed that the improvement of PhenomHM vs PhenomD to constrain the distance was increased by ~ 50 % (i.e., the posteriors of PhenomHM were narrower by 50% compared to PhenomD ) for the two detector network and for the HLV configuration, | ||
+ | * One caveat between those two runs was that for the HL run, the source was placed at a sky-position where the response was the maximum, but for the HLV run the source was at a sky-position where the response was about half of that. | ||
+ | * I wanted to check the effect of changing the inclination of the source on the recovery and to check for any biases on the posteriors and to check whether including a third detector would improve the results. | ||
+ | * With that in mind, I have started a set of runs for the BAM q4 & q8 non-spinning waveforms for two and three detector configuration, | ||
+ | * I've used the aLIGOzeroDetHighPower and aVIRGO PSD's for the runs. | ||
+ | * The base directory for all the run directories is at: __/ | ||
+ | |||
+ | ^ Simulation h5 file ^ Detector configuration | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HL | 0 | IMRPhenomD | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_0.0_M80_HL_PhenomD | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HL | 60 | IMRPhenomD | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_60.0_M80_HL_PhenomD | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HL | 90 | IMRPhenomD | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_90.0_M80_HL_PhenomD | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HL | 0 | IMRPhenomHM | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_0.0_M80_HL_PhenomHM | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HL | 60 | IMRPhenomHM | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_60.0_M80_HL_PhenomHM | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HL | 90 | IMRPhenomHM | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_90.0_M80_HL_PhenomHM | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HLV | 0 | IMRPhenomD | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_0.0_M80_HLV_PhenomD | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HLV | 60 | IMRPhenomD | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_60.0_M80_HLV_PhenomD | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HLV | 90 | IMRPhenomD | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_90.0_M80_HLV_PhenomD | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HLV | 0 | IMRPhenomHM | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_0.0_M80_HLV_PhenomHM | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HLV | 60 | IMRPhenomHM | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_60.0_M80_HLV_PhenomHM | Running | | | ||
+ | | q4a0_T_112_448_fix_scale_Lmax_4_Allm.h5 | HLV | 90 | IMRPhenomHM | 18/09/17 | BAM_q4a0a0_SNR_25_mode_lMax_4_inc_90.0_M80_HLV_PhenomHM | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HL | 0 | IMRPhenomD | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_0.0_M115_HL_PhenomD | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HL | 60 | IMRPhenomD | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_60.0_M115_HL_PhenomD | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HL | 90 | IMRPhenomD | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_90.0_M115_HL_PhenomD | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HL | 0 | IMRPhenomHM | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_0.0_M115_HL_PhenomHM | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HL | 60 | IMRPhenomHM | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_60.0_M115_HL_PhenomHM | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HL | 90 | IMRPhenomHM | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_90.0_M115_HL_PhenomHM | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HLV | 0 | IMRPhenomD | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_0.0_M115_HLV_PhenomD | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HLV | 60 | IMRPhenomD | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_60.0_M115_HLV_PhenomD | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HLV | 90 | IMRPhenomD | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_90.0_M115_HLV_PhenomD | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HLV | 0 | IMRPhenomHM | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_0.0_M115_HLV_PhenomHM | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HLV | 60 | IMRPhenomHM | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_60.0_M115_HLV_PhenomHM | Running | | | ||
+ | | q8a0a0_T_112_588n768_fix_scale_Lmax_4_Allm.h5 | HLV | 90 | IMRPhenomHM | 18/09/17 | BAM_q8a0a0_SNR_25_mode_lMax_4_inc_90.0_M115_HLV_PhenomHM | Running | | |
imrphenomhm_pe_study.1505476034.txt.gz · Last modified: 2017/09/15 11:47 by chinmay.kalaghatgi@LIGO.ORG