Hannu Parviainen, Instituto de Astrofísica de Canarias
Last updated: 22.06.2017
The notebooks in this directory are used mainly for the visualisation of the results obtained with the $W80ROOT/bin/fit script.
The fit script can be ran either as
fit --passband PB --nights NN --approach APP --n-threads 1 --n-walkers 800 --de-n-iterations 2500 --de-update-interval 100 --de-save-interval 100 --mc-n-iterations 15000 --mc-update-interval 200 --mc-save-interval 1000 --mc-thin 200 --mc-n-runs 5 --do-mc --use-ldtk
or (using bash)
for i in {1..5}; fit --passband PB --nights NN --approach APP --n-threads 1 --n-walkers 800 --de-n-iterations 2500 --de-update-interval 100 --de-save-interval 100 --mc-n-iterations 15000 --mc-update-interval 200 --mc-save-interval 1000 --mc-thin 200 --do-mc --use-ldtk; done
where PB is the passband in [nb, K, Na]; NN chooses the nights to use from [1, 2, 12]; and APP chooces the modeling approach from [abs, dw, dwr]. The first approach should work fine in theory, but there appears to be a memory leak in the code somewhere, which will eventually lead to a crash. The second approach is better until I find and fix the leak.
The code currently implements three modelling approaches
ABS: Direct model with GP systematicsDW: Divide-by-white model with parametric systematicsDWR: Divide-by-white model with GP systematicsThese approaches are implemented as classes in modules lpfsd, lpfsr, lpfsrr for single nights, and lpfmd, lpfmr, and lpfmrr for multiple nights. The LPFSD is a subclass of LPF, and LPFSR and LPFSRR are subclasses of LPFSD.