Hi Troels, Apart from the list of trivialities to fix (http://article.gmane.org/gmane.science.nmr.relax.devel/6345), any changes you make from now on should be in the trunk, or a new branch if it is disruptive. You're disp_spin_speed branch is done :) Cheers, Edward On 18 June 2014 09:41, <tlinnet@xxxxxxxxxxxxx> wrote:
Author: tlinnet Date: Wed Jun 18 09:41:11 2014 New Revision: 24065 URL: http://svn.gna.org/viewcvs/relax?rev=24065&view=rev Log: Made changes to the dir argument of systemtest Relax_disp.test_r1rho_kjaergaard. This is to prepare for: sr #3124 (https://gna.org/support/?3124): Grace graphs production for R1rho analysis with R2_eff as function of Omega_eff sr #3138 (https://gna.org/support/?3138): Interpolating theta through spin-lock offset [Omega], rather than spin-lock field strength [w1] This is also to test an expected bug, if R1 is not loaded. Task #7807 (https://gna.org/task/index.php?7807): Speed-up of dispersion models for Clustered analysis. Modified: branches/disp_spin_speed/test_suite/system_tests/relax_disp.py [This mail would be too long, it was shortened to contain the URLs only.] Modified: branches/disp_spin_speed/test_suite/system_tests/relax_disp.py URL: http://svn.gna.org/viewcvs/relax/branches/disp_spin_speed/test_suite/system_tests/relax_disp.py?rev=24065&r1=24064&r2=24065&view=diff _______________________________________________ relax (http://www.nmr-relax.com) This is the relax-commits mailing list relax-commits@xxxxxxx To unsubscribe from this list, get a password reminder, or change your subscription options, visit the list information page at https://mail.gna.org/listinfo/relax-commits