price@neverland:~/pfs/drp_stella (tickets/PIPE2D-290=) $ git sub
commit 4415c44ee44de4e2ef7f8b53e6601c5be889187d
Author: Paul Price <price@astro.princeton.edu>
Date:   Thu Sep 13 14:32:15 2018 -0400

    remove SWIG bindings
    
    We're using pybind11 now. How have these managed to stick around so long?

 python/pfs/drp/stella/stellaLib.i | 152 --------------------------------------
 1 file changed, 152 deletions(-)

commit 80bdd284fd72c1c9e1e6337415e0bf9660cdd54f
Author: Paul Price <price@astro.princeton.edu>
Date:   Thu Sep 13 14:53:40 2018 -0400

    DetectorMap: strip throughput
    
    A single value per fiber isn't sufficient to characterise the throughput
    as a function of wavelength for each fiber. We'll do this in the flat-field
    instead of carrying it around here.

 include/pfs/drp/stella/DetectorMap.h             | 25 +---------
 python/pfs/drp/stella/constructFiberTraceTask.py | 62 ------------------------
 python/pfs/drp/stella/detectorMap.cc             | 27 +++--------
 python/pfs/drp/stella/detectorMapContinued.py    | 16 +-----
 python/pfs/drp/stella/extractSpectraTask.py      |  1 -
 src/DetectorMap.cc                               | 45 +----------------
 tests/test_DetectorMap.py                        | 32 ++++--------
 7 files changed, 20 insertions(+), 188 deletions(-)

commit 0b76eff8b900b509d7250d98e3c08414b1c383ee
Author: Paul Price <price@astro.princeton.edu>
Date:   Tue Oct 2 21:34:44 2018 +0000

    FiberTraceSet: add extractSpectra method
    
    That's why you have a FiberTrace, right? So let's add a method to do that.

 python/pfs/drp/stella/fiberTracesContinued.py | 29 +++++++++++++++++++++++++++
 1 file changed, 29 insertions(+)

commit 7ccc5150684ca409f821866d3f1625ecb8362c5a
Author: Paul Price <price@astro.princeton.edu>
Date:   Tue Oct 2 21:37:28 2018 +0000

    refactor flat field normalisation
    
    Previously, each fiber was independently normalised, which means
    that flux calibrating one doesn't allow you to flux calibrate
    anything else (well, we have a throughput measurement in the
    DetectorMap, but that's not a function of wavelength). Instead,
    normalise all fibers to the mean spectrum of the fibers.
    This keeps the fibers tied together.

 python/pfs/drp/stella/constructFiberFlatTask.py | 115 +++++++++++++-----------
 1 file changed, 61 insertions(+), 54 deletions(-)

commit 2801f730a15e1ab95cc21f169c174ad259f129de
Author: Paul Price <price@astro.princeton.edu>
Date:   Tue Oct 2 21:36:06 2018 -0400

    make some files flake8-clean

 python/pfs/drp/stella/constructFiberTraceTask.py | 2 --
 python/pfs/drp/stella/detectorMapContinued.py    | 3 +--
 python/pfs/drp/stella/spectraContinued.py        | 4 ++--
 3 files changed, 3 insertions(+), 6 deletions(-)