From c9f7fe1993b169bc4a76dc596ac79192fa8363e0 Mon Sep 17 00:00:00 2001 From: ozerov_d Date: Wed, 6 Sep 2023 15:34:55 +0200 Subject: [PATCH] Update README.md --- README.md | 6 +++--- 1 file changed, 3 insertions(+), 3 deletions(-) diff --git a/README.md b/README.md index 4606435..f77477c 100644 --- a/README.md +++ b/README.md @@ -37,12 +37,12 @@ Automatic Processing tool can also be installed from scratch (put this to the pl $ git clone https://gitlab.psi.ch/sf-daq/ap.git # or via ssh with # git clone git@gitlab.psi.ch:sf-daq/ap.git ``` -Needed conda environment can be sourced/used from the common place. In case new conda environment is needed, please install following packages in that conda: +Needed conda environment can be sourced/used from the common place. In case new conda environment is needed, please install following packages in that environment: ``` gspread numpy matplotlib ``` -In case of installation from source, so different location of the code and conda environment - change correspondingly line in scripts/env_setup.sh +In case of installation from source, so different location of the code and conda environment - change correspondingly lines in [env_setup.sh](#config_env_setup) file ## Configuration files @@ -68,7 +68,7 @@ run9977 0.09413 ``` (for runs 9988 and 9977 - 9.212cm and 9.413cm will be used as detector distance, for all other runs a default value of 9.369cm will be used) -### env_setup.sh +### env_setup.sh During preparation [step](#usage1) this file should be filled (manually) with the proper values for the beamline name(alvra or bernina or ..), pgroup name (p12345), DETECTOR_NAME (JF17T16V01) used in experiment, THRESHOLD_INDEXING (can be changed, adapted, in run_index.sh file, see latter) and LOGBOOK (url to google spreadsheet which will be used for automatic filling) ### run_index.sh