S240422ed S240422ed
cbc-workflow-er16-o4b
Current version: 585cabf6
recorded 2026-06-11 00:45 UTC
v3
Metadata
Summary
- Instruments
- H1,L1,V1
- ADVOK state
- ✓ True
- False-alarm rate (FAR)
- 1.55×10⁻⁶
- Astrophysical probability (p_astro) classification
- 0.002
Info
Details
- Notes
- ""
All remaining fields
- id
- 22249
GraceDB
Key fields
- Instruments
- H1,L1,V1
- ADVOK state
- ✓ True
- False-alarm rate (FAR)
- 1.55×10⁻⁶
- Astrophysical probability (p_astro) classification
- 0.002
Details
- Notes
- ""
| Event identifier | Pipeline | State | GPS time | False-alarm rate (FAR) | Network signal-to-noise ratio | Astrophysical probability | Binary black-hole probability | Binary neutron-star probability | Neutron-star–black-hole probability | Primary mass | Secondary mass |
|---|---|---|---|---|---|---|---|---|---|---|---|
| G631838 | gstlal | neighbor | 1397856931.40732 | 1.55×10⁻⁶ | 1.04×10¹ | — | — | — | — | 3.44×10⁰ | 1.19×10⁰ |
| G476954 | gstlal | preferred | 1397856931.417261 | 3.1×10⁻¹³ | 1.02×10¹ | 1 | 0 | 0 | 1 | 3.44×10⁰ | 1.19×10⁰ |
All remaining fields
- id
- 186850
- label
- ""
- h1 snr
- 4.8080893
- l1 snr
- 8.5831728
- v1 snr
- —
- k1 snr
- —
- g1 snr
- —
- spin 1z
- 0.75796872
- spin 2z
- 0.75796872
- has ns
- 1.0
- has remnant
- 1.0
- has mass gap
- 0.37249934216110686
- pipeline has ns
- —
- pipeline has remnant
- —
- pipeline has mass gap
- —
- xml
- https://gracedb.ligo.org/api/v2/events/G631838/files/coinc.xml
- source classification
- ""
- skymap
- https://gracedb.ligo.org/api/v2/events/G631838/files/bayestar.multiorder.fits
- early warning
- ✗ False
- search type
- offline
- catalog number
- 5
- catalog version
- 25.0
- in offline catalog
- ✓ True
- notes
- ""
- id
- 186851
- label
- ""
- h1 snr
- 4.8088651
- l1 snr
- 8.5834236
- v1 snr
- 2.7788472
- k1 snr
- —
- g1 snr
- —
- spin 1z
- 0.75796875
- spin 2z
- 0.75796875
- has ns
- 1.0
- has remnant
- 1.0
- has mass gap
- 0.4592902600687565
- pipeline has ns
- —
- pipeline has remnant
- —
- pipeline has mass gap
- —
- xml
- https://gracedb.ligo.org/api/v2/events/G476954/files/coinc.xml
- source classification
- https://gracedb.ligo.org/api/v2/events/G476954/files/gstlal.p_astro.json
- skymap
- https://gracedb.ligo.org/api/v2/events/G476954/files/bayestar.multiorder.fits
- early warning
- ✗ False
- search type
- low latency
- catalog number
- ""
- catalog version
- —
- in offline catalog
- ✗ False
- notes
- ""
- id
- 22249
- last update
- —
Parameter estimation (PE)
Details
- Parameter-estimation status
- ongoing
- Analysts
- id: 7, name: aaron.zimmerman, id: 82, name: anuj.mishra, id: 98, name: sylvia.biscoveanu, +6 more
- Reviewers
- id: 7, name: aaron.zimmerman, id: 98, name: sylvia.biscoveanu, id: 120, name: cjhaster
- Notes
- NSBH candidate that was downranked offline
| Result identifier | Inference software | Waveform approximant | Run status | Review status | Analysts | Reviewers | Deprecated |
|---|---|---|---|---|---|---|---|
| online | bilby | IMRPhenomPv2 | Complete | ongoing | Empty list | Empty list | ✗ False |
| Exp1 | bilby | IMRPhenomPv2 | Complete | pass | Empty list | Empty list | ✓ True |
| Exp3 | bilby | IMRPhenomPv2 | Complete | pass | Empty list | Empty list | ✗ False |
| EXP0 | bilby | IMRPhenomPv2 | Complete | pass | Empty list | Empty list | ✓ True |
| EXP2 | bilby | IMRPhenomPv2 | Complete | pass | Empty list | Empty list | ✓ True |
| Exp10 | bilby | IMRPhenomNSBH | Complete | fail | Empty list | Empty list | ✓ True |
| Exp4 | bilby | IMRPhenomNSBH | Complete | fail | Empty list | Empty list | ✓ True |
| Exp7 | bilby | SEOBNRv4_ROM_NRTidalv2_NSBH | Complete | fail | Empty list | Empty list | ✓ True |
| Exp8 | bilby | IMRPhenomPv2 | Complete | pass | Empty list | Empty list | ✗ False |
| Exp9 | bilby | IMRPhenomPv2 | Complete | fail | Empty list | Empty list | ✓ True |
| Exp11 | bilby | IMRPhenomXPHM | Complete | pass | Empty list | Empty list | ✗ False |
| Exp12 | bilby | IMRPhenomNSBH | Complete | fail | Empty list | Empty list | ✓ True |
| Exp6 | parallel_bilby | SEOBNRv5PHM | "" | pass | Empty list | Empty list | ✗ False |
| Exp14 | bilby | IMRPhenomPv2_NRTidalv2 | Complete | fail | Empty list | Empty list | ✓ True |
| Exp13 | bilby | IMRPhenomXPHM | Complete | pass | Empty list | Empty list | ✗ False |
| Exp16 | bilby | IMRPhenomXPHM | Complete | pass | Empty list | Empty list | ✗ False |
| Exp15 | bilby | IMRPhenomPv2_NRTidalv2 | Complete | pass | Empty list | Empty list | ✗ False |
All remaining fields
- id
- 129700
- config file
-
- id
- 15630
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/online/bilby/G476954_config_complete.ini
- md5 sum
- 3d6aa1af76e14fb9d3c91261472e9adb
- date last modified
- 2024-04-22T14:41:40+10:00
- public html
- ""
- result file
-
- id
- 15631
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/online/bilby/final_result/G476954_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 61c18fe0698aa4e510a39cf7ce686745
- date last modified
- 2024-04-22T15:25:05+10:00
- public html
- ""
- pesummary result file
-
- id
- 15632
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/online/summary/samples/posterior_samples.h5
- md5 sum
- 73434a3b90e15c2cd904ee86a23b5a70
- date last modified
- 2024-04-22T16:16:18+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/online/summary/home.html
- publications
- ""
- notes
- Automatic online PE run succeeded Results copied from /home/pe.o4/O4b/S240422ed/online/bilby Results rail against lower q prior bound High primary spin also suspicious, attempting manual followup When this file is updated add the contents as a comment on the relevant git issue. Instructions can be found [here](https://git.ligo.org/pe/O4/o4b-rota/-/wikis/Review-instructions). Perform a review of the online result and assess if it is sufficent for sending a skymap.
- id
- 129701
- config file
-
- id
- 15633
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp1/bilby/G476954_config_complete.ini
- md5 sum
- c9631afc6fd776c7914da6710155d6ae
- date last modified
- 2024-04-22T16:13:22+10:00
- public html
- ""
- result file
-
- id
- 15634
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp1/bilby/final_result/G476954_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 7fb91ae16423fe12807727cb3ea8885d
- date last modified
- 2024-04-22T17:52:39+10:00
- public html
- ""
- pesummary result file
-
- id
- 15637
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp1/summary/samples/posterior_samples.h5
- md5 sum
- bb5e4a2df89e81180d8740259f3e25a8
- date last modified
- 2024-04-22T19:15:44+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp1/summary/home.html
- publications
- ""
- notes
- Expanded q prior resolves the peak in q, possible gentle railing Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/FreqCut0 Manual run with wider q priors and higher flow flow of 30 Hz in L1 didn't seem to make a difference
- id
- 129702
- config file
-
- id
- 15635
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp3/bilby/Exp3_config_complete.ini
- md5 sum
- e832a1816f1e0ac8ff217f48d285b9bf
- date last modified
- 2024-04-22T16:21:25+10:00
- public html
- ""
- result file
-
- id
- 15636
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp3/bilby/final_result/Exp3_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 4290b9a40369d8101c34c35b4723b88e
- date last modified
- 2024-04-22T18:01:40+10:00
- public html
- ""
- pesummary result file
-
- id
- 15638
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp3/summary/samples/posterior_samples.h5
- md5 sum
- ef09eb9e15a4557dec0f4eb7d965b89b
- date last modified
- 2024-04-22T19:23:55+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp3/summary/home.html
- publications
- ""
- notes
- This run used to release skymap update Expanded q prior resolves the peak in q, possible gentle railing Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/Exp3 Manual run with wider q priors and higher flow flow of 30 Hz in L1 and 25 Hz in H1 didn't seem to make a difference
- id
- 129703
- config file
-
- id
- 15639
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/EXP0/bilby/G476954_config_complete.ini
- md5 sum
- 36e142d1950b78dba419da9073a959ff
- date last modified
- 2024-04-22T16:09:56+10:00
- public html
- ""
- result file
-
- id
- 15640
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/EXP0/bilby/final_result/G476954_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- af8aba69b2b77502c48a4dbb78ccd4a5
- date last modified
- 2024-04-22T22:12:07+10:00
- public html
- ""
- pesummary result file
-
- id
- 15641
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/EXP0/summary/samples/posterior_samples.h5
- md5 sum
- eede24d9d2e4cc80c6eaaee45a9db767
- date last modified
- 2024-04-23T00:17:45+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/EXP0/summary/home.html
- publications
- ""
- notes
- Run used fLow=20Hz for H1 and V1, and fLow=25Hz for L1. This configuration gives generally consistent results with the other EXP0-3 runs Results copied from /home/carl-johan.haster/projects/O4/S240422ed/EXP0 Expanded q prior resolves the peak in q, possible gentle railing Manual run with wider q priors and higher flow in L1
- id
- 129704
- config file
-
- id
- 15642
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/EXP2/bilby/G476954_config_complete.ini
- md5 sum
- 898a9be3ab0d48dce3c2a57bd85ec107
- date last modified
- 2024-04-22T16:18:09+10:00
- public html
- ""
- result file
-
- id
- 15643
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/EXP2/bilby/final_result/G476954_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- e42b2c546d027b8e4873d0666acc33c4
- date last modified
- 2024-04-22T21:22:36+10:00
- public html
- ""
- pesummary result file
-
- id
- 15644
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/EXP2/summary/samples/posterior_samples.h5
- md5 sum
- f35623116c0bd50ea7bbd45996ec1d05
- date last modified
- 2024-04-23T00:25:52+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/EXP2/summary/home.html
- publications
- ""
- notes
- Expanded q prior resolves the peak in q, possible gentle railing Run used fLow=20Hz for V1, and fLow=25Hz for L1 and H1. This configuration gives generally consistent results with the other EXP0-3 runs Results copied from /home/carl-johan.haster/projects/O4/S240422ed/EXP2 Manual run with wider q priors and higher flow in L1 and H1
- id
- 129705
- config file
-
- id
- 15645
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp10/bilby/Exp10_config_complete.ini
- md5 sum
- befbded954101edd22ae0d944eadc745
- date last modified
- 2024-04-24T10:03:08+10:00
- public html
- ""
- result file
-
- id
- 15646
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp10/bilby/final_result/Exp10_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 0827c0c0175fb6d7f96e3e197f33928c
- date last modified
- 2024-04-24T10:05:28+10:00
- public html
- ""
- pesummary result file
-
- id
- 15647
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp10/summary/samples/posterior_samples.h5
- md5 sum
- d0fa8779abf4ed3147178bc8fe069fc7
- date last modified
- 2024-04-24T19:28:09+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp10/summary/home.html
- publications
- ""
- notes
- flow of 30 Hz in L1 and 25 Hz in H1 didn't seem to make a difference This run used to release skymap update Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/Exp3 Manual run with wider q priors and higher flow Expanded q prior resolves the peak in q, possible gentle railing now railing in mass ratio and bimodal in chirp mass no overlap with original chirp mass posterior same as Exp4 but wider chirp mass prior from 1.5 - 2 Msun
- id
- 129706
- config file
-
- id
- 15648
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp4/bilby/Exp4_config_complete.ini
- md5 sum
- 942573b23b5b3151e096f7790d4d3ef2
- date last modified
- 2024-04-23T19:21:20+10:00
- public html
- ""
- result file
-
- id
- 15649
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp4/bilby/final_result/Exp4_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 207c12d47b2685d798c92a36596cdb08
- date last modified
- 2024-04-23T19:23:21+10:00
- public html
- ""
- pesummary result file
-
- id
- 15650
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp4/summary/samples/posterior_samples.h5
- md5 sum
- bc8ed8fea5955fbf0591b39dac4d37e2
- date last modified
- 2024-04-24T19:18:10+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp4/summary/home.html
- publications
- ""
- notes
- Railing strongly in chirp mass due to spin restrictions Using chirp mass prior recommended by configurator for Exp3 Relative binning likelihood, fmin=30 for all IFOs IMRPhenomNSBH run with a_1 < 0.5, a_2 < 0.05
- id
- 129707
- config file
-
- id
- 15651
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp7/bilby/Exp7_config_complete.ini
- md5 sum
- 20ddbdae675ac754cc3ee7eff7294a7b
- date last modified
- 2024-04-24T06:44:24+10:00
- public html
- ""
- result file
-
- id
- 15652
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp7/bilby/final_result/Exp7_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 4de7ff20a473595bfa0350b033d992dd
- date last modified
- 2024-04-24T06:46:24+10:00
- public html
- ""
- pesummary result file
-
- id
- 15653
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp7/summary/samples/posterior_samples.h5
- md5 sum
- f3d9c5fb89742346aa9fc4ab789bece5
- date last modified
- 2024-04-24T19:25:30+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp7/summary/home.html
- publications
- ""
- notes
- Using chirp mass prior recommended by configurator for Exp3 Relative binning likelihood, fmin=30 for all IFOs SEOBNR NSBH run with a_1 < 0.5, a_2 < 0.09 Railing in chirp mass due to spin restrictions SEOBNR NSBH run with a_1 < 0.9, a_2 < 0.05
- id
- 129708
- config file
-
- id
- 15654
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp8/bilby/Exp8_config_complete.ini
- md5 sum
- 1a67f9349ff6b2a92dcb1f9621dc67dc
- date last modified
- 2024-04-23T08:54:45+10:00
- public html
- ""
- result file
-
- id
- 15655
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp8/bilby/final_result/Exp8_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- abb991325edddafdde2233882e0f5e8b
- date last modified
- 2024-04-23T10:45:38+10:00
- public html
- ""
- pesummary result file
-
- id
- 15658
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp8/summary/samples/posterior_samples.h5
- md5 sum
- 76eed55f79ef1bbe04e0c5a92229375a
- date last modified
- 2024-04-24T19:43:42+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp8/summary/home.html
- publications
- ""
- notes
- flow of 30 Hz in L1 and 25 Hz in H1 didn't seem to make a difference This run used to release skymap update Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/Exp3 Manual run with wider q priors and higher flow Expanded q prior resolves the peak in q, possible gentle railing same as Exp3 but with coherence test seemingly no signal recovered in Hanford
- id
- 129710
- config file
-
- id
- 15656
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp9/bilby/Exp9_config_complete.ini
- md5 sum
- 7d02171aeb1af01e47cb87e30311816b
- date last modified
- 2024-04-23T13:26:06+10:00
- public html
- ""
- result file
-
- id
- 15657
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp9/bilby/final_result/Exp9_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 8f07800e44a85a192c7a33c725e8dc06
- date last modified
- 2024-04-23T13:28:35+10:00
- public html
- ""
- pesummary result file
-
- id
- 15659
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp9/summary/samples/posterior_samples.h5
- md5 sum
- 9a673f83ca1868e61a2b1ea4060a46e0
- date last modified
- 2024-04-25T05:18:13+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp9/summary/home.html
- publications
- ""
- notes
- flow of 30 Hz in L1 and 25 Hz in H1 didn't seem to make a difference This run used to release skymap update Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/Exp3 Manual run with wider q priors and higher flow Expanded q prior resolves the peak in q, possible gentle railing same as Exp3 except for flow and coherence test flow '{H1:20, L1:60, V1:20}' railing against lower chirp mass bound in Livingston
- id
- 129712
- config file
-
- id
- 15660
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp11/bilby/Exp11_config_complete.ini
- md5 sum
- f520474576a8b90b76f756b09e9044f7
- date last modified
- 2024-04-25T08:13:12+10:00
- public html
- ""
- result file
-
- id
- 15661
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp11/bilby/final_result/Exp11_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- d7218254cf0e208a605e49b6eec7e602
- date last modified
- 2024-04-25T08:16:56+10:00
- public html
- ""
- pesummary result file
-
- id
- 15662
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp11/summary/samples/posterior_samples.h5
- md5 sum
- e6d05bc85791757ee00c2f00467c4686
- date last modified
- 2024-04-26T08:22:31+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp11/summary/home.html
- publications
- ""
- notes
- Same frequency settings as Exp3 but 256s duration IMRPhenomXPHM with MultiBanding likelihood Posteriors agree with IMRPhenomPv2 results
- id
- 129713
- config file
-
- id
- 15663
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp12/bilby/Exp12_config_complete.ini
- md5 sum
- f545a440e0c967d249585acda060104d
- date last modified
- 2024-04-26T00:43:25+10:00
- public html
- ""
- result file
-
- id
- 15664
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp12/bilby/final_result/Exp12_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 071efa577a50365d89eafd9d6bd3669e
- date last modified
- 2024-04-26T00:45:37+10:00
- public html
- ""
- pesummary result file
-
- id
- 15665
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp12/summary/samples/posterior_samples.h5
- md5 sum
- 005871228782be1fc13d40e36661a661
- date last modified
- 2024-04-26T09:18:54+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp12/summary/home.html
- publications
- ""
- notes
- Posteriors seem well-converged but are entirely discrepant with the high-spin BBH runs Copy of Exp4 but with wider chirp mass and mass ratio priors Reweighting to the regular GW likelihood reveals a failure of the relative binning likelihood, with only one effective sample
- id
- 129715
- config file
-
- id
- 15666
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp6/parallel_bilby/Exp6_config_complete.ini
- md5 sum
- d7a535647dbe929cfc6f26e4693566eb
- date last modified
- 2024-04-23T09:52:07+10:00
- public html
- ""
- result file
- —
- pesummary result file
- —
- bayeswave
- Empty list
- pesummary page url
- ""
- publications
- ""
- notes
- Same frequency settings as Exp3 but 256s duration SEOBNRv5PHM with parallel-bilby Posteriors agree with IMRPhenomPv2 and XPHM results
- id
- 129717
- config file
-
- id
- 15667
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp14/bilby/Exp14_config_complete.ini
- md5 sum
- d0a2f2597e40585cffd3a031bbfede8b
- date last modified
- 2024-05-08T06:17:10+10:00
- public html
- ""
- result file
-
- id
- 15668
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp14/bilby/final_result/Exp14_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 89031e89db607157357452daf47468ab
- date last modified
- 2024-05-08T06:18:35+10:00
- public html
- ""
- pesummary result file
-
- id
- 15669
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp14/summary/samples/posterior_samples.h5
- md5 sum
- 4d45e70651c0fb0f60558c0b50c449b3
- date last modified
- 2024-05-08T22:16:13+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp14/summary/home.html
- publications
- ""
- notes
- Chirp mass posterior is railing against the lower end while the primary spin magnitude a_1 is railing against the upper end. Thus, due to the restrictions on spins, it did not lead to fruitful posteriors. Same settings as Exp13 but with "IMRPhenomPv2_NRTidalv2" waveform approximant keeping lambda_1=0. We also used broader chirp mass and mass ratio priors.
- id
- 129720
- config file
-
- id
- 15670
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp13/bilby/Exp13_config_complete.ini
- md5 sum
- ec7e94aea7fac4a50198f2761d254609
- date last modified
- 2024-04-29T14:14:46+10:00
- public html
- ""
- result file
-
- id
- 15671
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp13/bilby/final_result/Exp13_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- a341c2dda27b4853889834d0686553a8
- date last modified
- 2024-04-29T14:16:47+10:00
- public html
- ""
- pesummary result file
-
- id
- 15672
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp13/summary/samples/posterior_samples.h5
- md5 sum
- 3b580b0dc06807ce65d17d97bd38491f
- date last modified
- 2024-04-30T01:23:55+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp13/summary/home.html
- publications
- ""
- notes
- Same settings as Exp11 but with a higher maximum-frequency of 3584 Hz. Posteriors agree with IMRPhenomPv2 results
- id
- 129722
- config file
-
- id
- 15673
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp16/bilby/Exp16_config_complete.ini
- md5 sum
- e9359e260cdaba21ac8aaee451be4b38
- date last modified
- 2024-05-01T22:22:23+10:00
- public html
- ""
- result file
-
- id
- 15674
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp16/bilby/final_result/Exp16_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- 90f61a468218e12215526079d2f250d3
- date last modified
- 2024-05-01T20:43:30+10:00
- public html
- ""
- pesummary result file
-
- id
- 15675
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp16/summary/samples/posterior_samples.h5
- md5 sum
- 578be2806165ca1ecfb15345b2113f1c
- date last modified
- 2024-05-01T23:19:58+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp16/summary/home.html
- publications
- ""
- notes
- Same settings as Exp11 but with a higher maximum-frequency of 3584 Hz. Posteriors agree with IMRPhenomPv2 results Reference frequency used is 100 Hz. Posteriors mostly agree with IMRPhenomPv2 results, except the posterior of the secondary spin magnitude give more weightage to higher values. Same settings as Exp13 but with broader chirp mass and mass ratio priors.
- id
- 129724
- config file
-
- id
- 15676
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp15/bilby/Exp15_config_complete.ini
- md5 sum
- ec932ad6a41322d4d53e5397d373df16
- date last modified
- 2024-05-14T14:18:01+10:00
- public html
- ""
- result file
-
- id
- 15677
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp15/bilby/final_result/Exp15_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- md5 sum
- b040581905ccaaa12a5bee36729fae24
- date last modified
- 2024-05-14T14:22:49+10:00
- public html
- ""
- pesummary result file
-
- id
- 15678
- path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp15/summary/samples/posterior_samples.h5
- md5 sum
- 4e4cae3d8e04083b3948a90fb69a17dc
- date last modified
- 2024-05-14T16:16:54+10:00
- public html
- ""
- bayeswave
- Empty list
- pesummary page url
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp15/summary/home.html
- publications
- ""
- notes
- IMRPhenomPv2_NRTidalv2 with relative binning likelihood, lambda_1=0 256s duration, fmin=30 Hz, fmax=3584 Hz Posteriors agree with BBH waveform results, lambda_2 uninformative
- id
- 22249
- illustrative result
- N/A
- skymap release result
- N/A
- safe sampling rate
- 4096.0
- safe lower chirp mass
- —
- safe upper chirp mass
- —
- safe lower primary mass
- —
- safe upper primary mass
- —
- safe lower secondary mass
- —
- safe upper secondary mass
- —
- safe lower mass ratio
- 0.05
- safe upper luminosity distance
- —
- safe geocent time
- —
- configurator duration
- —
- configurator minimum frequency
- —
- configurator maximum frequency
- —
Tests of general relativity (TGR)
Details
- Notes
- ""
All remaining fields
- id
- 22252
- imrct analyses
- Empty list
- tiger analyses
- Empty list
- fti analyses
- Empty list
- pcatgr analyses
- Empty list
- pseobrd analyses
- Empty list
- pyring analyses
- Empty list
- pol analyses
- Empty list
- mdr analyses
- Empty list
- sim analyses
- Empty list
- ssb analyses
- Empty list
- bhm analyses
- Empty list
- losa analyses
- Empty list
- sma analyses
- Empty list
- echoes cwb analyses
- Empty list
- residuals analyses
- Empty list
- unmodeled echoes analyses
- Empty list
- qnm rational filter analyses
- Empty list
- modeled echoes analyses
- Empty list
Lensing
All remaining fields
- Companion superevent
- Empty list
- Singlet analysis identifier
- Empty list
- id
- 22252
Detector characterisation (Detchar)
Details
- Notes
- ""
All remaining fields
- id
- 22252
- recommended detectors
-
- Item 1
-
- id
- 11017
- uid
- H1
- recommended minimum frequency
- 20.0
- recommended maximum frequency
- —
- recommended start time
- —
- recommended end time
- —
- recommended channel
- H1:DCS-CALIB_STRAIN_CLEAN_AR01
- glitch mitigation status
- not required
- frame type
- H1_HOFT_AR01
- frame file
- ""
- notes
- This event is really close to LLO going into observing. PE configurator wants a 512s window, but there's too much noise at the beginning of the segment. So I need to recommend a 256s window. There's also isolated glitches in LLO below 30 Hz
- Item 2
-
- id
- 11018
- uid
- L1
- recommended minimum frequency
- 30.0
- recommended maximum frequency
- —
- recommended start time
- —
- recommended end time
- —
- recommended channel
- L1:DCS-CALIB_STRAIN_CLEAN_AR01
- glitch mitigation status
- not required
- frame type
- L1_HOFT_AR01
- frame file
- ""
- notes
- This event is really close to LLO going into observing. PE configurator wants a 512s window, but there's too much noise at the beginning of the segment. So I need to recommend a 256s window. There's also isolated glitches in LLO below 30 Hz
- Item 3
-
- id
- 11019
- uid
- V1
- recommended minimum frequency
- 20.0
- recommended maximum frequency
- —
- recommended start time
- —
- recommended end time
- —
- recommended channel
- V1:Hrec_hoftRepro1AR_16384Hz
- glitch mitigation status
- not required
- frame type
- HoftAR1U02
- frame file
- ""
- notes
- This event is really close to LLO going into observing. PE configurator wants a 512s window, but there's too much noise at the beginning of the segment. So I need to recommend a 256s window. There's also isolated glitches in LLO below 30 Hz
- dqr results
-
- Item 1
-
- id
- 4650
- dqr file
-
- id
- 15683
- path
- CIT:/home/dqr/public_html/o4dqr/online/events/202404/S240422ed/index.html
- md5 sum
- 7ebce20f32b748e79f4f4b1a3659be0d
- date last modified
- 2024-04-25T04:12:32+10:00
- public html
- https://ldas-jobs.ligo.caltech.edu/~dqr/o4dqr/online/events/202404/S240422ed/index.html
- uid
- review status
- pass
- validation result
- pass
- validation notes
- ""
- notes
- ""
- analysts
-
- Item 1
-
- id
- 8
- name
- Derek Davis
- Item 2
-
- id
- 9
- name
- Laura Nuttall
- Item 3
-
- id
- 11
- name
- Siddharth Soni
- Item 4
-
- id
- 12
- name
- derek.davis@ligo.org
- Item 5
-
- id
- 13
- name
- laura.nuttall@port.ac.uk
- Item 6
-
- id
- 15
- name
- siddharth.soni@ligo.org
- Item 7
-
- id
- 46
- name
- Adrian Helmling-Cornell
- Item 8
-
- id
- 56
- name
- Sophie Hourihane
- Item 9
-
- id
- 57
- name
- sophie.hourihane@ligo.org
- Item 10
-
- id
- 58
- name
- Francesco Di Renzo
- Item 11
-
- id
- 59
- name
- f.di-renzo@ip2i.in2p3.fr
- Item 12
-
- id
- 239
- name
- adrian.helmlingcornell@gmail.com
- reviewers
-
- Item 1
-
- id
- 9
- name
- Laura Nuttall
- Item 2
-
- id
- 13
- name
- laura.nuttall@port.ac.uk
- status
- complete
- recommended duration
- 256.0
- participating detectors
- H1,L1,V1
Extreme matter
Details
- Notes
- ""
All remaining fields
- id
- 22252
- analyses
- Empty list
Cosmology
Details
- Notes
- ""
All remaining fields
- id
- 22252
- counterparts
- Empty list
- runs
- Empty list
- preferred low latency skymap
- https://gracedb.ligo.org/api/v2/events/G476954/files/bayestar.multiorder.fits
Rapid neutron-star parameter estimation (RNP)
All remaining fields
- id
- 22252
- runs
- Empty list
Catalogue tracking
Details
- Notes
- ""
All remaining fields
- id
- 18797
- pe statuses
-
- Item 1
-
- id
- 16548
- uid
- IMRPhenomXPHM
- review status
- unstarted
- finalized
- ✗ False
- is designated illustrative result
- ✗ False
- corresponding pe uid
- NoCorrespondingResultFound
- notes
- No production results satisfying request available, using best rota analysis instead
- search statuses
-
- Item 1
-
- id
- 96508
- uid
- gstlal
- review status
- unstarted
- finalized
- ✗ False
- chunk
- 0.0
- notes
- ""
- Item 2
-
- id
- 96509
- uid
- pycbc
- review status
- unstarted
- finalized
- ✗ False
- chunk
- 0.0
- notes
- ""
Publications
All remaining fields
- id
- 22249
- papers
- ""
Additional metadata: id
All remaining fields
- id
- 22249
Additional metadata: sname
All remaining fields
- sname
- S240422ed
Additional metadata: commit sha
All remaining fields
- commit sha
- 585cabf6c647081f8649197c52a62052a40df764
Additional metadata: commit timestamp
All remaining fields
- commit timestamp
- 2026-06-11T10:45:11+10:00
Additional metadata: is current
All remaining fields
- is current
- ✓ True
Additional metadata: schema version
All remaining fields
- schema version
- v3
Additional metadata: raw payload
All remaining fields
- raw payload
-
- Info
-
- Notes
- Empty list
- Labels
- Empty list
- SchemaVersion
- v3
- Sname
- S240422ed
- GraceDB
-
- ADVOK
- ✓ True
- Events
-
- Item 1
-
- FAR
- 1.548775838256943e-06
- UID
- G631838
- XML
- https://gracedb.ligo.org/api/v2/events/G631838/files/coinc.xml
- H1SNR
- 4.8080893
- HasNS
- 1.0
- L1SNR
- 8.5831728
- Mass1
- 3.4434683
- Mass2
- 1.1861781
- Notes
- Empty list
- State
- neighbor
- Skymap
- https://gracedb.ligo.org/api/v2/events/G631838/files/bayestar.multiorder.fits
- Spin1z
- 0.75796872
- Spin2z
- 0.75796872
- GPSTime
- 1397856931.40732
- Pipeline
- gstlal
- HasMassGap
- 0.37249934216110686
- HasRemnant
- 1.0
- NetworkSNR
- 10.38626030737269
- SearchType
- offline
- EarlyWarning
- ✗ False
- CatalogNumber
- 5
- CatalogVersion
- 25
- InOfflineCatalog
- ✓ True
- Item 2
-
- FAR
- 3.095258031034583e-13
- UID
- G476954
- XML
- https://gracedb.ligo.org/api/v2/events/G476954/files/coinc.xml
- Pbbh
- 7.235379608546062e-16
- Pbns
- 1.0351710548560264e-16
- H1SNR
- 4.8088651
- HasNS
- 1.0
- L1SNR
- 8.5834236
- Mass1
- 3.4434683
- Mass2
- 1.1861781
- Notes
- Empty list
- Pnsbh
- 0.999986151010447
- State
- preferred
- V1SNR
- 2.7788472
- Pastro
- 0.9999861510104477
- Skymap
- https://gracedb.ligo.org/api/v2/events/G476954/files/bayestar.multiorder.fits
- Spin1z
- 0.75796875
- Spin2z
- 0.75796875
- GPSTime
- 1397856931.417261
- Pipeline
- gstlal
- HasMassGap
- 0.4592902600687565
- HasRemnant
- 1.0
- NetworkSNR
- 10.22361658639324
- SearchType
- low latency
- EarlyWarning
- ✗ False
- InOfflineCatalog
- ✗ False
- SourceClassification
- https://gracedb.ligo.org/api/v2/events/G476954/files/gstlal.p_astro.json
- LastUpdate
- 2026-06-10 17:44:56.080932
- Instruments
- H1,L1,V1
- SupereventFAR
- 1.548775838256943e-06
- SupereventPastro
- 0.0018508024604060314
- Lensing
-
- SingletAnalyses
- —
- MultipletAnalyses
- —
- Cosmology
-
- Notes
- Empty list
- Counterparts
- Empty list
- PreferredLowLatencySkymap
- https://gracedb.ligo.org/api/v2/events/G476954/files/bayestar.multiorder.fits
- CosmologyRunsUsingThisSuperevent
- Empty list
- TestingGR
-
- Notes
- Empty list
- BHMAnalyses
- Empty list
- FTIAnalyses
- Empty list
- MDRAnalyses
- Empty list
- POLAnalyses
- Empty list
- SIMAnalyses
- Empty list
- SMAAnalyses
- Empty list
- SSBAnalyses
- Empty list
- LOSAAnalyses
- Empty list
- IMRCTAnalyses
- Empty list
- TIGERAnalyses
- Empty list
- PCATGRAnalyses
- Empty list
- PYRINGAnalyses
- Empty list
- PSEOBRDAnalyses
- Empty list
- EchoesCWBAnalyses
- Empty list
- ResidualsAnalyses
- Empty list
- ModeledEchoesAnalyses
- Empty list
- UnmodeledEchoesAnalyses
- Empty list
- QNMRationalFilterAnalyses
- Empty list
- Publications
-
- Papers
- Empty list
- ExtremeMatter
-
- Analyses
- Empty list
- CatalogTracking
-
- Notes
- Empty list
- SearchResultStatuses
-
- Item 1
-
- UID
- gstlal
- Chunk
- 0
- Notes
- Empty list
- Finalized
- ✗ False
- ReviewStatus
- unstarted
- Item 2
-
- UID
- pycbc
- Chunk
- 0
- Notes
- Empty list
- Finalized
- ✗ False
- ReviewStatus
- unstarted
- ParameterEstimationStatuses
-
- Item 1
-
- UID
- IMRPhenomXPHM
- Notes
-
- Item 1
- No production results satisfying request available, using best rota analysis instead
- Finalized
- ✗ False
- ReviewStatus
- unstarted
- CorrespondingPEUID
- NoCorrespondingResultFound
- IsDesignatedIllustrativeResult
- ✗ False
- ParameterEstimation
-
- Notes
-
- Item 1
- NSBH candidate that was downranked offline
- Status
- ongoing
- Results
-
- Item 1
-
- UID
- online
- Notes
-
- Item 1
- Automatic online PE run succeeded
- Item 2
- Results copied from /home/pe.o4/O4b/S240422ed/online/bilby
- Item 3
- Results rail against lower q prior bound
- Item 4
- High primary spin also suspicious, attempting manual followup
- Item 5
- When this file is updated add the contents as a comment on the relevant git issue.
- Item 6
- Instructions can be found [here](https://git.ligo.org/pe/O4/o4b-rota/-/wikis/Review-instructions).
- Item 7
- Perform a review of the online result and assess if it is sufficent for sending a skymap.
- RunStatus
- complete
- ConfigFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/online/bilby/G476954_config_complete.ini
- MD5Sum
- 3d6aa1af76e14fb9d3c91261472e9adb
- DateLastModified
- 2024/04/22 14:41:40
- Deprecated
- ✗ False
- ResultFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/online/bilby/final_result/G476954_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- MD5Sum
- 61c18fe0698aa4e510a39cf7ce686745
- DateLastModified
- 2024/04/22 15:25:05
- Publications
- Empty list
- ReviewStatus
- ongoing
- PESummaryPageURL
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/online/summary/home.html
- InferenceSoftware
- bilby
- PESummaryResultFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/online/summary/samples/posterior_samples.h5
- MD5Sum
- 73434a3b90e15c2cd904ee86a23b5a70
- DateLastModified
- 2024/04/22 16:16:18
- WaveformApproximant
- IMRPhenomPv2
- Item 2
-
- UID
- Exp1
- Notes
-
- Item 1
- Expanded q prior resolves the peak in q, possible gentle railing
- Item 2
- Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/FreqCut0
- Item 3
- Manual run with wider q priors and higher flow
- Item 4
- flow of 30 Hz in L1 didn't seem to make a difference
- RunStatus
- complete
- ConfigFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp1/bilby/G476954_config_complete.ini
- MD5Sum
- c9631afc6fd776c7914da6710155d6ae
- DateLastModified
- 2024/04/22 16:13:22
- Deprecated
- ✓ True
- ResultFile
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- Manual run with wider q priors and higher flow
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- Results copied from /home/carl-johan.haster/projects/O4/S240422ed/EXP0
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- Expanded q prior resolves the peak in q, possible gentle railing
- Item 4
- Manual run with wider q priors and higher flow in L1
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- Expanded q prior resolves the peak in q, possible gentle railing
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- Results copied from /home/carl-johan.haster/projects/O4/S240422ed/EXP2
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- Manual run with wider q priors and higher flow in L1 and H1
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-
- Item 1
- flow of 30 Hz in L1 and 25 Hz in H1 didn't seem to make a difference
- Item 2
- This run used to release skymap update
- Item 3
- Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/Exp3
- Item 4
- Manual run with wider q priors and higher flow
- Item 5
- Expanded q prior resolves the peak in q, possible gentle railing
- Item 6
- now railing in mass ratio and bimodal in chirp mass
- Item 7
- no overlap with original chirp mass posterior
- Item 8
- same as Exp4 but wider chirp mass prior from 1.5 - 2 Msun
- RunStatus
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- Railing strongly in chirp mass due to spin restrictions
- Item 2
- Using chirp mass prior recommended by configurator for Exp3
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- Item 4
- IMRPhenomNSBH run with a_1 < 0.5, a_2 < 0.05
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- Relative binning likelihood, fmin=30 for all IFOs
- Item 3
- SEOBNR NSBH run with a_1 < 0.5, a_2 < 0.09
- Item 4
- Railing in chirp mass due to spin restrictions
- Item 5
- SEOBNR NSBH run with a_1 < 0.9, a_2 < 0.05
- RunStatus
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- Item 9
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-
- Item 1
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- Item 2
- This run used to release skymap update
- Item 3
- Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/Exp3
- Item 4
- Manual run with wider q priors and higher flow
- Item 5
- Expanded q prior resolves the peak in q, possible gentle railing
- Item 6
- same as Exp3 but with coherence test
- Item 7
- seemingly no signal recovered in Hanford
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-
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- Notes
-
- Item 1
- flow of 30 Hz in L1 and 25 Hz in H1 didn't seem to make a difference
- Item 2
- This run used to release skymap update
- Item 3
- Results copied from /home/aaron.zimmerman/working/O4/PE/S240422ed/Exp3
- Item 4
- Manual run with wider q priors and higher flow
- Item 5
- Expanded q prior resolves the peak in q, possible gentle railing
- Item 6
- same as Exp3 except for flow and coherence test
- Item 7
- flow '{H1:20, L1:60, V1:20}'
- Item 8
- railing against lower chirp mass bound in Livingston
- RunStatus
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- Item 11
-
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- Notes
-
- Item 1
- Same frequency settings as Exp3 but 256s duration
- Item 2
- IMRPhenomXPHM with MultiBanding likelihood
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- Posteriors agree with IMRPhenomPv2 results
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- Item 12
-
- UID
- Exp12
- Notes
-
- Item 1
- Posteriors seem well-converged but are entirely discrepant with the high-spin BBH runs
- Item 2
- Copy of Exp4 but with wider chirp mass and mass ratio priors
- Item 3
- Reweighting to the regular GW likelihood reveals a failure of the relative binning likelihood, with only one effective sample
- RunStatus
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-
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- Item 13
-
- UID
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- Notes
-
- Item 1
- Same frequency settings as Exp3 but 256s duration
- Item 2
- SEOBNRv5PHM with parallel-bilby
- Item 3
- Posteriors agree with IMRPhenomPv2 and XPHM results
- ConfigFile
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- Item 14
-
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- Notes
-
- Item 1
- Chirp mass posterior is railing against the lower end while the primary spin magnitude a_1 is railing against the upper end. Thus, due to the restrictions on spins, it did not lead to fruitful posteriors.
- Item 2
- Same settings as Exp13 but with "IMRPhenomPv2_NRTidalv2" waveform approximant keeping lambda_1=0.
- Item 3
- We also used broader chirp mass and mass ratio priors.
- RunStatus
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- Path
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- Item 15
-
- UID
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- Notes
-
- Item 1
- Same settings as Exp11 but with a higher maximum-frequency of 3584 Hz.
- Item 2
- Posteriors agree with IMRPhenomPv2 results
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- Item 16
-
- UID
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- Notes
-
- Item 1
- Same settings as Exp11 but with a higher maximum-frequency of 3584 Hz.
- Item 2
- Posteriors agree with IMRPhenomPv2 results
- Item 3
- Reference frequency used is 100 Hz.
- Item 4
- Posteriors mostly agree with IMRPhenomPv2 results, except the posterior of the secondary spin magnitude give more weightage to higher values.
- Item 5
- Same settings as Exp13 but with broader chirp mass and mass ratio priors.
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- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp16/summary/home.html
- InferenceSoftware
- bilby
- PESummaryResultFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp16/summary/samples/posterior_samples.h5
- MD5Sum
- 578be2806165ca1ecfb15345b2113f1c
- DateLastModified
- 2024/05/01 23:19:58
- WaveformApproximant
- IMRPhenomXPHM
- Item 17
-
- UID
- Exp15
- Notes
-
- Item 1
- IMRPhenomPv2_NRTidalv2 with relative binning likelihood, lambda_1=0
- Item 2
- 256s duration, fmin=30 Hz, fmax=3584 Hz
- Item 3
- Posteriors agree with BBH waveform results, lambda_2 uninformative
- RunStatus
- complete
- ConfigFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp15/bilby/Exp15_config_complete.ini
- MD5Sum
- ec932ad6a41322d4d53e5397d373df16
- DateLastModified
- 2024/05/14 14:18:01
- Deprecated
- ✗ False
- ResultFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp15/bilby/final_result/Exp15_data0_1397856931-4073198_analysis_H1L1V1_merge_result.hdf5
- MD5Sum
- b040581905ccaaa12a5bee36729fae24
- DateLastModified
- 2024/05/14 14:22:49
- Publications
- Empty list
- ReviewStatus
- pass
- PESummaryPageURL
- https://ldas-jobs.ligo.caltech.edu/~pe.o4/O4b/S240422ed/Exp15/summary/home.html
- InferenceSoftware
- bilby
- PESummaryResultFile
-
- Path
- CIT:/home/pe.o4/public_html/O4b/S240422ed/Exp15/summary/samples/posterior_samples.h5
- MD5Sum
- 4e4cae3d8e04083b3948a90fb69a17dc
- DateLastModified
- 2024/05/14 16:16:54
- WaveformApproximant
- IMRPhenomPv2_NRTidalv2
- Analysts
-
- Item 1
- anna.heffernan
- Item 2
- hector.estelles
- Item 3
- cjhaster
- Item 4
- surabhi.sachdev
- Item 5
- aaron.zimmerman
- Item 6
- hsiang-yu.huang
- Item 7
- ben.patterson
- Item 8
- anuj.mishra
- Item 9
- sylvia.biscoveanu
- Reviewers
-
- Item 1
- sylvia.biscoveanu
- Item 2
- cjhaster
- Item 3
- aaron.zimmerman
- SafeSamplingRate
- 4096.0
- IllustrativeResult
- N/A
- SafeLowerMassRatio
- 0.05
- SkymapReleaseResult
- N/A
- RatesAndPopulations
-
- RnPRunsUsingThisSuperevent
- Empty list
- DetectorCharacterization
-
- Notes
-
- Item 1
- ""
- Status
- complete
- Analysts
-
- Item 1
- Adrian Helmling-Cornell
- Item 2
- adrian.helmlingcornell@gmail.com
- Item 3
- Derek Davis
- Item 4
- derek.davis@ligo.org
- Item 5
- Sophie Hourihane
- Item 6
- sophie.hourihane@ligo.org
- Item 7
- Laura Nuttall
- Item 8
- laura.nuttall@port.ac.uk
- Item 9
- Francesco Di Renzo
- Item 10
- f.di-renzo@ip2i.in2p3.fr
- Item 11
- Siddharth Soni
- Item 12
- siddharth.soni@ligo.org
- Reviewers
-
- Item 1
- Laura Nuttall
- Item 2
- laura.nuttall@port.ac.uk
- DQRResults
-
- Item 1
-
- UID
- Notes
-
- Item 1
- ""
- DQRFile
-
- Path
- CIT:/home/dqr/public_html/o4dqr/online/events/202404/S240422ed/index.html
- MD5Sum
- 7ebce20f32b748e79f4f4b1a3659be0d
- PublicHTML
- https://ldas-jobs.ligo.caltech.edu/~dqr/o4dqr/online/events/202404/S240422ed/index.html
- DateLastModified
- 2024/04/25 04:12:32
- ReviewStatus
- pass
- ValidationNotes
-
- Item 1
- ""
- ValidationResult
- pass
- RecommendedDuration
- 256.0
- RecommendedDetectors
-
- Item 1
-
- UID
- H1
- Notes
-
- Item 1
- This event is really close to LLO going into observing. PE configurator wants a 512s window, but there's too much noise at the beginning of the segment. So I need to recommend a 256s window. There's also isolated glitches in LLO below 30 Hz
- FrameType
- H1_HOFT_AR01
- RecommendedChannel
- H1:DCS-CALIB_STRAIN_CLEAN_AR01
- GlitchMitigationStatus
- not required
- RecommendedMinimumFrequency
- 20
- Item 2
-
- UID
- L1
- Notes
-
- Item 1
- This event is really close to LLO going into observing. PE configurator wants a 512s window, but there's too much noise at the beginning of the segment. So I need to recommend a 256s window. There's also isolated glitches in LLO below 30 Hz
- FrameType
- L1_HOFT_AR01
- RecommendedChannel
- L1:DCS-CALIB_STRAIN_CLEAN_AR01
- GlitchMitigationStatus
- not required
- RecommendedMinimumFrequency
- 30
- Item 3
-
- UID
- V1
- Notes
-
- Item 1
- This event is really close to LLO going into observing. PE configurator wants a 512s window, but there's too much noise at the beginning of the segment. So I need to recommend a 256s window. There's also isolated glitches in LLO below 30 Hz
- FrameType
- HoftAR1U02
- RecommendedChannel
- V1:Hrec_hoftRepro1AR_16384Hz
- GlitchMitigationStatus
- not required
- RecommendedMinimumFrequency
- 20
- ParticipatingDetectors
-
- Item 1
- H1
- Item 2
- L1
- Item 3
- V1
Additional metadata: created at
All remaining fields
- created at
- 2026-07-28T10:46:08.880369+10:00
Additional metadata: updated at
All remaining fields
- updated at
- 2026-07-28T10:46:08.880374+10:00