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Merge branch 'develop' into slitorder_fix
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profxj authored Nov 19, 2021
2 parents fdefa5c + 4adf05c commit f179a75
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1 change: 1 addition & 0 deletions CHANGES.rst
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- uses dither offeset recorded in the header as default slitmask_offset,
but the user can provide the maskdef_id of a slit with a bright object that can trace the offset.
- improvements in the frame typing
- Implements new Mark4 detector for Keck/LRISr (aka keck_lris_red_mark4)


1.6.0 (1 Oct 2021)
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19 changes: 14 additions & 5 deletions doc/lris.rst
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Expand Up @@ -82,8 +82,17 @@ very blue.
keck_lris_red
=============

Taking Calibrations for LRISr
=============================
Detectors
+++++++++

There have been 3 (or is it 4?!) generations of detectors
in the LRISr camera. The original is named `keck_lris_red_orig`,
the LBNL detectors (2kx4k) are `keck_lris_red` and the newest
Mark4 detector is `keck_lris_red_mark4`.

For the latter (Mark4), the wavelengths have been incorporated for the
R400 grating only so far but the arxiv solutions from the LBNL detector
may work ok. Check the outputs!

LRISr Default Settings
++++++++++++++++++++++
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settings trace slits pca params [3,2,1,0]

Known issues
++++++++++++
============

LRISb Slit Edges
----------------
++++++++++++++++

When observing in long-slit mode, PypeIt might set the slit incorrectly
for detector 2. This may occur if the counts from the flat field
Expand All @@ -123,7 +132,7 @@ Here is an example for the PypeIt file::
This will force a slit onto the detector for reduction.

Multi-slit
----------
++++++++++

The code may identify a 'ghost' slit in empty detector real
estate if your mask does not fill most of the field. Be prepared
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