You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
Include a fix for when no edges are detected in EdgeTraceSet by
adding the bound_detector parameter. Most instruments have a
default of bound_detector = False meaning that the code will skip
processing any detector where no slit edges are found. Some
instuments set the default to be bound_detector = True because the
slit edges always or often fall off the edge of the detector (i.e.,
the detector is fully illuminated). These instruments are currently mmt_mmirs, mmt_bluechannel, not_alfosc, and shane_kast; note
that some gemini_gmos data in the DevSuite require bound_detector=True, as well.
Improved wavelength template for DEIMOS gratings: 600ZD, 830G.
Added new ArI, KrI, NeI, XeI arc lines.
PypeIt can now compute arc line FWHM from the lines themselves. This
is controlled by a new parset, fwhm_fromlines, which is set to
False by default, except for DEIMOS.
Added a development document about the DEIMOS wavelength calibration.
Limit reduction to detectors 3 and 7 when DEIMOS LVM mask is used
(other detectors are empty)
Add wavelength RMS to SpecObj. This is an update of the datamodel to
1.3.3
Add Bok B&C spectrograph
Add pypeit_obslog script that simple compiles and prints metadata
from a set of fits files needed by pypeit to run.
Change PypeItSetup.from_file_root to require the output path to
write the vanilla pypeit file. If no path is provided, the object is
instatiated without creating any output.
Fixed bug in sensitivity function code adressing issue #747. Revamped sensitivity
function completely to compute zeropoints and throughput. Enhanced sensfunc.py QA.
Added MOSFIRE QL script.
Added support for VLT/SINFONI K 25mas (0.8x0.8 arcsec FOV) platescale
Updated docs for differencing imaging sky subtraction.