Commit c0028df9 authored by Médéric Boquien's avatar Médéric Boquien
Browse files

Fix a crash in the computation of the rectangular periodic SFH with Numpy 1.12

parent a11ed956
......@@ -23,6 +23,7 @@
- The Herschel passbands only included the filter. Now they include the full throughput of the instrument. Flux differences are expected to be no more than 1%. (Médéric Boquien)
- The `dustatt_powerlaw` module indicated that the Milky Way bump has an amplitude of 3. This is only valid for the `dustatt_calzleit` module. As `dustatt_powerlaw` is normalised to A(V) rather than E(B-V) for `dustatt_calzleit`, the bump is a factor Rv larger. A more reasonable value is now given. (Médéric Boquien)
- The correction of the χ² for the upper limits now properly takes into account earlier changes intended to reduce memory usage and speed up the analysis. This prevents a crash. (Médéric Boquien)
- Fix a crash in the computation of the rectangular periodic SFH with Numpy 1.12. (Médéric Boquien)
### Optimised
- By default the MKL library created many threads for each for the parallel processes. Not only was this not necessary as a high-level parallelisation already exists, but it generated a strong oversubscription on the CPU and on the RAM. The slowdown was over a factor of ~2 in some cases. Now we mandate KML to use only 1 thread fo each process. (Médéric Boquien & Yannick Roehlly)
......@@ -85,7 +85,7 @@ class SfhPeriodic(SedModule):
elif self.type_bursts == 2:
burst = np.zeros_like(time_grid)
burst[:self.tau_bursts+1] = 1.
burst[:int(self.tau_bursts)+1] = 1.
raise Exception("Burst type {} unknown.".format(self.type_bursts))
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