Closed fjebaker closed 1 year ago
Merging #74 (86d5c15) into main (ec031bb) will increase coverage by
2.66%
. The diff coverage is60.34%
.
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@@ Coverage Diff @@
## main #74 +/- ##
==========================================
+ Coverage 69.02% 71.69% +2.66%
==========================================
Files 43 44 +1
Lines 1485 1512 +27
==========================================
+ Hits 1025 1084 +59
+ Misses 460 428 -32
Impacted Files | Coverage Δ | |
---|---|---|
src/point-functions.jl | 52.38% <0.00%> (ø) |
|
src/corona-to-disc/disc-profiles.jl | 65.46% <50.00%> (+1.18%) |
:arrow_up: |
src/transfer-functions/transfer-functions-2d.jl | 67.30% <60.00%> (-16.03%) |
:arrow_down: |
src/line-profiles.jl | 78.26% <78.57%> (-21.74%) |
:arrow_down: |
...ransfer-functions/cunningham-transfer-functions.jl | 97.33% <100.00%> (ø) |
|
src/transfer-functions/precision-solvers.jl | 63.82% <100.00%> (ø) |
|
src/utils.jl | 100.00% <100.00%> (ø) |
|
src/metrics/johannsen-psaltis-ad.jl | 100.00% <0.00%> (+5.55%) |
:arrow_up: |
... and 4 more |
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Cleaned up a number of bugs, including what was discussed in #71 (thread).
Started drafting the disc profiles API so we can use all sorts of fun emissivity profiles for the accretion disc models when calculating e.g. lag transfers or line profiles. This is very early days yet and no new user API is exposed in this PR.
Added more tests and fixed some inference issues.