Merge branch 'master' of https://github.com/igrins/plp

README.md

@@ -2,19 +2,7 @@
 
 # IGRINS Pipeline Package
 
-IGRINS pipeline package is currently in active development. Version 1, that was originally developed by Prof. Soojong Pak's team at Kyung Hee University (KHU), is deprecated and is not recommended to use. While the version 2 of the pipeline is still in active development, it is encouraged that you try this version.
-
-- https://github.com/igrins/plp/releases
-
-## Version 2
-
-While the original pipeline by KHU's team works to some extent, there
-are things that need to be fixed/improved/extended. A new version of
-pipeline (version 2) is being actively developed by the pipeline team
-at KASI (led by Dr. Jae-Joon Lee) in close collaboration with KHU's
-team.
-
-The new pipeline is designed to produce decent quality of processed
+The IGRINS PLP is designed to produce decent quality of processed
 data of all the observing data without (or minimum) human interaction. It was also
 designed to be adaptable for a real time processing during the
 observing run.
@@ -25,24 +13,28 @@ observatories/instruments. In most cases, the recipe needs to be set
 and recorded in the header (or log) when the observation is
 executed. Unfortunately, this is not properly done. Therefore, to run
 the pipeline, you should have an input file describing which recipe
-should be used to which data sets. 
+should be used to which data sets.
+
+IGRINS pipeline package is currently in active development. Version 3 is the latest version and is recommended for use for reducing data from the McDonald 2.7m, LDT/DCT, and Gemini-South telescopes.  Version 2 will still work for those who need it.  Version 1, that was originally developed by Prof. Soojong Pak's team at Kyung Hee University (KHU), is deprecated and is not recommended to use.  Versions 2-3 were developed by the pipeline team at KASI (led by Dr. Jae-Joon Lee) in close collaboration with KHU's team.  Additional development and testing for v3 has been carried out by Kyle Kaplan and Erica Sawczynec at the University of Texas at Austin Department of Astronomy.
 
-The page below briefly describes how to run the pipeline version 2.
 
- - https://github.com/igrins/plp/wiki/How-to-run-pipeline
 
+## Downloads
 
-## Version 1
+- https://github.com/igrins/plp/releases
 
-This is the original pipeline that has developed by Prof. Soojong
-Pak's team at Kyung Hee University (KHU). We recommend users to use the version 2 instead of this.
+## Documentation
 
-The version 1 pipeline is described in the following publication.
+- https://github.com/igrins/plp/wiki/
 
-- http://adsabs.harvard.edu/abs/2014AdSpR..53.1647S
+## The Raw & Reduced IGRINS Spectral Archive (RRISA)
+IGRINS data is made publically availiable through the The Raw & Reduced IGRINS Spectral Archive (RRISA).  The current version of RRISA (v1) uses the IGRINS PLP v2 for it's data reductions.  The raw data are also availiable for RRISA for those who want to perform their own data reduction with the IGRINGS PLP.
 
-More information about this version can be found from the link below.
+- RRISA v1: https://igrinscontact.github.io
 
-- http://irlab.khu.ac.kr/~igrins/
 
+## Publications
+
+The version 1 pipeline is described in the following publication.
+- http://adsabs.harvard.edu/abs/2014AdSpR..53.1647S