Skip to content

Commit 412e1b6

Browse files
(ノ◕ヮ◕)ノ adhere to mighty pre-commit
1 parent 2c4725c commit 412e1b6

File tree

1 file changed

+3
-3
lines changed

1 file changed

+3
-3
lines changed

README.md

Lines changed: 3 additions & 3 deletions
Original file line numberDiff line numberDiff line change
@@ -5,15 +5,15 @@ This is the lightcurves repository. Check it out: [![Open In Colab](https://cola
55
See here for scientific application of this code:
66
https://pos.sissa.it/395/868
77

8-
## LC.py
8+
## lc.py
99
Initialize a LightCurve object based on time, flux and flux_error.
1010
Study its Bayesian block representation (based on Scargle et al. 2013 https://ui.adsabs.harvard.edu/abs/2013arXiv1304.2818S/abstract ).<br>
1111
Characterize flares (start, peak, end time) with the HOP algorithm (following Meyer et al. 2019 https://ui.adsabs.harvard.edu/abs/2019ApJ...877...39M/abstract ). There are four different methods to define flares (baseline, half, flip, sharp) as illustrated in the Jupyter Notebook.
1212

13-
## HOP.py
13+
## hop.py
1414
Initialize a Hopject to consider parameters of an individual flare.
1515

16-
## LC_Set
16+
## lc_set
1717
Initialize a (large) sample of light curves to study the distribution of flare parameters whithin that sample.<br>
1818

1919

0 commit comments

Comments
 (0)