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@kbwestfall kbwestfall released this 20 Sep 14:44
· 2014 commits to release since this release
1.14.0
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Dependency Changes

  • Main dependency bumps: numpy>=1.22, matplotlib>=3.7, ginga>=4.1.1,
    qtpy>=2.0.1

Functionality/Performance Improvements and Additions

  • Improvements to wavelength grids and masking in coadd routines.

  • Refactored coadding routines to work with lists to support coadding
    data from different setups.

  • Sensitivity function models can now be computed relative to the
    flat-field spectrum.

  • Improvements in 2D coaddition

    • Fix a bug in pypeit_setup_coadd2d for the output file name of
      the .coadd2d file
    • Added possibility to specify more than one Science folder in
      pypeit_setup_coadd2d
    • Now only_slits parameter in pypeit_coadd_2dspec includes
      the detector number (similar to slitspatnum)
    • Added exclude_slits parameter in pypeit_coadd_2dspec to
      exclude specific slits
    • Fix wrong RA and Dec for 2D coadded serendips

  • Allow wavelength calibrations for specific slits/orders to be redone
    (instead of adopting the value from a processed calibration frame);
    see new redo_slits parameter.

Instrument-specific Updates

  • Adds/Improves support for Gemini/GNIRS (IFU), Keck/KCRM, Keck/ESI,
    MDM/Modspec, Keck/HIRES, JWST

  • HIRES wavelength solution improvements galore

  • Improvements for Keck/LRIS

    • Generated wavelength templates for all the LRIS grism & grating
    • Added FeAr line list
    • Improved calibration association and frame typing
    • Improved and added documentation
    • Changes to metadata.py including commenting out, in the pypeit
      file, files that have frametype None (this prevent run_pypeit
      to crash)
    • Added a function check_spectrograph() (currently only defined
      for LRIS), that checks (during pypeit_setup) if the selected
      spectrograph is the corrected one for the data used.

Script Changes

  • Added a script to convert a wavelength solution into something that
    can be placed in the reid archive.
  • Store user-generated wavelength solution in pypeit cache

Datamodel Changes

  • Changed calibration frame naming as an attempt to avoid very long
    names for files with many calibration groups. Sequential numbers are
    reduced to a range; e.g., '0-1-2-3-4' becomes '0+4' and
    '3-5-6-10-11-12-15-18-19' becomes '3-5+6-10+12-15-18+19'
  • Instrumental FWHM map is calculated and output in Calibrations and
    spec1d files.

Under-the-hood Improvements

  • Change how masking is dealt with in extraction to fix a bug in how
    masks were being treated for echelle data
  • Refactored function that loads wavelength calibration line lists

Bug Fixes

  • Hotfix for GTC/OSIRIS lamp list

  • Hotfix for Arc1D stats annotations on the QA

  • Hotfix for metadata:

    • correctly set config_independent_frames when multiple
      configurations are being setup
    • support lists in config_independent_frames

  • Hotfix for rebin (speed-up and conserves flux)

  • Hotfix for skysub regions GUI that used np.bool

  • Hotfix to stop pypeit_setup from crashing on data from lbt_luci1,
    lbt_luci2, magellan_fire, magellan_fire_long, p200_tspec, or
    vlt_sinfoni.

  • Hotfix to set BPM for each type of calibration file.

  • Fixed a bug in echelle coadding where the wrong coadded spectra were
    being used in final stacks.

  • Fix a bug in spectrograph.select_detectors, where a list of
    slitspatnum could not be used.

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