Synthetic Observations of pre-merger BBH from the e-NOVAs
Here are some of the lightcurve and full energy spectrum from our publication. They are available to download, if you use them please cite the original papier from which they are from.In case you are interested in a different setup than the ones presented here, you can contact us as it might be part of a soon to be released set that could be upload ahead or we could, given time, produce such set.
BBH in a circular orbit
publication associated On the origin of the lump in circumbinary discs Raphael Mignon-Risse, Peggy Varniere, Fabien Casse, MNRAS, Volume 520, Issue 1, March 2023, Pages 1285-1295.
Looking at a fully characterized system
Here we look at the data for a fully determined system with the approximation that the system stays in a circular orbit for the entire observation. All the data are in the directory according to their parameters
| mass ratio | separation | inclination | total mass | LC/spectrum |
|---|---|---|---|---|
| 1 | 20 | 70 | 1e5 | LC and spectrum for M=1e5 q=1 b=20 incli=70 |
| 0.3 | 20 | 70 | 1e5 | LC and spectrum for M=1e5 q=0.3 b=20 incli=70 |
| 0.1 | 20 | 70 | 1e5 | LC and spectrum for M=1e5 q=0.1 b=20 incli=70 |
| 1 | 36 | 70 | 1e7 | LC and spectrum for M=1e7 q=1 b=36 incli=70 |
| 0.3 | 36 | 70 | 1e6 | LC and spectrum for M=1e6 q=0.3 b=36 incli=70 |
| 0.3 | 33 | 70 | 1e7 | LC and spectrum for M=1e7 q=0.3 b=33 incli=70 |
Looking for a particular lightcurve's behavior
As we are showing the lightcurve normalized, there is no mass dependency. Only in the energy spectrum does the mass appear.
Click on the chosen lightcurve to access the files to download for the different masses.
A look at the far zone
Raphaël Mignon-Risse, Peggy Varniere, Fabien Casse, MNRAS, Volume 519, Issue 2, February 2023, Pages 2848-2861.
The outer circumbinary disk exhibit the imprint of the gravitational wave passage, though at a very low level.
spectrum for M=1e10 q=1 chis=0.9 b=8 incli=60 spectrum for M=1e7 q=1 chis=0.9 b=8 incli=60 spectrum for M=1e5 q=1 chis=0.9 b=8 incli=60
spectrum for M=1e5 q=1 chis=0 b=8 incli=60 spectrum for M=1e5 q=0.3 chis=0 b=8 incli=60 spectrum for M=1e5 q=0.1 chis=0 b=8 incli=60