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
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