Open avivajpeyi opened 4 years ago
Dear Avi,
Thank you for your interest. I do not recover your plot when I download the
samples myself from the repository, please find attached the plot I get.
The culprits seem to be the transformations of the mass parameters. The
samples report mchirp
and eta
.
To be sure:
mchirp
is the detector-frame chirp mass, i.e.
mchirp = (1+z) (m1_sourcem2_source)0.6 / (m1_source+m2_source)0.2
where z is the cosmological redshift and m1_source, m2_source are the
source-frame component masses.
eta
is the symmetric mass ratio:
eta = m1*m2/(m1+m2)**2
Could you please double-check whether you are using these definitions? This said, if you still would like to have the PSDs let me know and I will be happy to provide them. Best regards, Javier
El lun, 30 nov 2020 a las 21:31, Avi Vajpeyi (notifications@github.com) escribió:
Hi @jroulet https://github.com/jroulet!
I tried plotting the LVC GW150914 posterior samples (obtained from GWOSC) against your GW150914 samples, and the results appear rather different: [image: test] https://user-images.githubusercontent.com/15642823/100689792-4e544f00-33d9-11eb-9c49-eb7ee08ce2c2.png
I was wondering -- could you upload your PSDs that you used for your analysis? Id like to try re-doing your analysis to better understand why the results are so different.
Thanks!
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Ah, I did not realise the samples headings were for
Correcting the above, I get:
(haven't calculated the z
values as they take a while to compute).
Would it still be possible to upload your PSDs?
Hi @jroulet!
I tried plotting the LVC GW150914 posterior samples (obtained from GWOSC) against your GW150914 samples, and the results appear rather different:
I was wondering -- could you upload your PSDs that you used for your analysis? Id like to try re-doing your analysis to better understand why the results are so different.
Thanks!