CHANGES

CHANGES.rst

@@ -1,23 +1,27 @@
-1.6.1dev
---------
+
+
+1.7.0 (19 Nov 2021)
+-------------------
 
 - Introduces pypeit_parse_calib_id script
-- Throw a warning if the chosen spectrograph has a header which does not match expectation
-- Pypeit can now read (currently for Keck DEIMOS only) the list of arc lamps from
-  the header and use it for wavelength calibration.
+- Throw a warning if the chosen spectrograph has a header which does not
+  match expectation
+- Pypeit can now read (currently for Keck DEIMOS only) the list of arc
+  lamps from the header and use it for wavelength calibration.
 - Allow one to restrict the wavelength range of the arxiv template
 - Set DEIMOS FWHM default to 10 pixels
-- Fixed a bug in HolyGrail that did not allow for sigdetect and rms_wavelength to be
-  slit dependent lists.
+- Fixed a bug in HolyGrail that did not allow for sigdetect and
+  rms_wavelength to be slit dependent lists.
 - Improvements for MOSFIRE:
     - uses slitmask info in the slit edge tracing
     - associates RA, Dec and Object name to each extracted object
-    - extracts undetected objects using the predicted position from slitmask info
-    - 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.
+    - extracts undetected objects using the predicted position from
+      slitmask info
+    - 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)
-
+- Implements new Mark4 detector for Keck/LRISr (aka keck_lris_red_mark4)
 
 1.6.0 (1 Oct 2021)
 ------------------