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author | glisse <glisse@636b058d-ea47-450e-bf9e-a15bfbe3eedb> | 2018-03-12 15:55:23 +0000 |
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committer | glisse <glisse@636b058d-ea47-450e-bf9e-a15bfbe3eedb> | 2018-03-12 15:55:23 +0000 |
commit | 11c9005fb1c9be03e208323a6933af66e87813a6 (patch) | |
tree | 2a2874fece353cbcd65dff026055cfdc0c69ec04 /src | |
parent | c1ddf3c7d276e946064c09c77b6969a71afaf41b (diff) |
git-svn-id: svn+ssh://scm.gforge.inria.fr/svnroot/gudhi/branches/sparserips-glisse@3278 636b058d-ea47-450e-bf9e-a15bfbe3eedb
Former-commit-id: 68262663f0fbeceef2a81929e42799479e7038f8
Diffstat (limited to 'src')
-rw-r--r-- | src/Rips_complex/doc/Intro_rips_complex.h | 6 |
1 files changed, 3 insertions, 3 deletions
diff --git a/src/Rips_complex/doc/Intro_rips_complex.h b/src/Rips_complex/doc/Intro_rips_complex.h index 909735cd..9cc58412 100644 --- a/src/Rips_complex/doc/Intro_rips_complex.h +++ b/src/Rips_complex/doc/Intro_rips_complex.h @@ -85,9 +85,9 @@ namespace rips_complex { * diagrams are at log-bottleneck distance at most \f$O(\epsilon)\f$). * * The sparse Rips filtration was introduced by Don Sheehy - * \cite sheehy13linear. We are using the version from \cite buchet16efficient - * (except that we multiply all filtration values by 2, to match the usual - * Rips complex), which proves a + * \cite sheehy13linear. We are using the version described in + * \cite buchet16efficient (except that we multiply all filtration values + * by 2, to match the usual Rips complex), which proves a * \f$\frac{1+\epsilon}{1-\epsilon}\f$-interleaving, although in practice the * error is usually smaller. * A more intuitive presentation of the idea is available in |