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Molecular dynamics by NMR data analysis
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SVN archive Commit Log
| Commit | Date | |
|---|---|---|
|
[r21376]
by
bugman
Added the scripting interface for cpmg_fit to the dispersion software comparison table in the manual. |
2013-11-04 10:55:05 | Tree |
|
[r21375]
by
bugman
Readded the accidentally deleted \clearpage command to keep the dispersion software table nicely formatted. |
2013-11-04 10:30:24 | Tree |
|
[r21374]
by
bugman
Updates for the TODO section of the dispersion chapter of the user manual. Some of the entries were rubbish! |
2013-11-04 10:29:19 | Tree |
|
[r21373]
by
bugman
Updated the GLOVE details in the dispersion software comparison table in the manual. |
2013-11-04 10:24:12 | Tree |
| 2013-11-04 10:20:26 | Tree | |
|
[r21371]
by
bugman
Added Dmitry Korzhnev's cpmg_fit software to the dispersion chapter of the manual. This is in the last section of that chapter and in the software comparison table. |
2013-11-04 10:13:35 | Tree |
|
[r21370]
by
bugman
Better organisation of the models by data type in the dispersion software comparison table in the manual. |
2013-11-04 10:00:21 | Tree |
|
[r21369]
by
bugman
Added a header comment to the grace2images.py script to explain its dependence on Grace. This is thanks to feedback from Nikolai Skrynnikov. |
2013-11-04 08:14:09 | Tree |
|
[r21368]
by
bugman
The dispersion target function num_disp_points structure is now variable. The number of points can now be different for each experiment type and each magnetic field strength. |
2013-10-31 19:50:20 | Tree |
|
[r21367]
by
bugman
The return_cpmg_frqs() and return_spin_lock_nu1() dispersion functions now return lists of lists of arrays. The dispersion data structures are now experiment and spectrometer frequency dependent. Therefore |
2013-10-31 19:35:54 | Tree |
