29.04.2013 Views

TESI DOCTORAL - La Salle

TESI DOCTORAL - La Salle

TESI DOCTORAL - La Salle

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

E.2. InternetAds data set<br />

φ (NMI)<br />

1<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0<br />

CSPA rb−cos−i2<br />

E λc<br />

λ 2 c<br />

λ 5 c<br />

λ 10<br />

c<br />

λ 15<br />

c<br />

λ 20<br />

c<br />

(a) CSPA<br />

φ (NMI)<br />

λ 30<br />

c<br />

1<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0<br />

λ 40<br />

c<br />

λ 50<br />

c<br />

λ 75<br />

c<br />

φ (NMI)<br />

1<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0<br />

ALSAD rb−cos−i2<br />

E λc<br />

λ 2 c<br />

λ 5 c<br />

λ 10<br />

c<br />

λ 15<br />

c<br />

λ 20<br />

c<br />

λ 30<br />

c<br />

(e) ALSAD<br />

λ 40<br />

c<br />

EAC rb−cos−i2<br />

E λc<br />

λ 2 c<br />

λ 5 c<br />

λ 10<br />

c<br />

λ 15<br />

c<br />

λ 20<br />

c<br />

(b) EAC<br />

λ 50<br />

c<br />

λ 75<br />

c<br />

φ (NMI)<br />

λ 30<br />

c<br />

1<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0<br />

λ 40<br />

c<br />

λ 50<br />

c<br />

λ 75<br />

c<br />

φ (NMI)<br />

1<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0<br />

KMSAD rb−cos−i2<br />

E λc<br />

λ 2 c<br />

λ 5 c<br />

λ 10<br />

c<br />

λ 15<br />

c<br />

λ 20<br />

c<br />

λ 30<br />

c<br />

(f) KMSAD<br />

λ 40<br />

c<br />

HGPA rb−cos−i2<br />

E λc<br />

λ 2 c<br />

λ 5 c<br />

λ 10<br />

c<br />

λ 15<br />

c<br />

λ 20<br />

c<br />

(c) HGPA<br />

λ 50<br />

c<br />

λ 75<br />

c<br />

φ (NMI)<br />

λ 30<br />

c<br />

1<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0<br />

λ 40<br />

c<br />

λ 50<br />

c<br />

λ 75<br />

c<br />

φ (NMI)<br />

1<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0<br />

SLSAD rb−cos−i2<br />

E λc<br />

λ 2 c<br />

λ 5 c<br />

λ 10<br />

c<br />

λ 15<br />

c<br />

λ 20<br />

c<br />

λ 30<br />

c<br />

(g) SLSAD<br />

λ 40<br />

c<br />

MCLA rb−cos−i2<br />

E λc<br />

λ 2 c<br />

λ 5 c<br />

λ 10<br />

c<br />

λ 15<br />

c<br />

λ 20<br />

c<br />

(d) MCLA<br />

Figure E.8: φ (NMI) boxplots of the self-refined intermodal consensus clustering solutions<br />

using the rb-cos-i2 algorithm on the CAL500 data set.<br />

E.2 InternetAds data set<br />

In the following paragraphs, the results corresponding to the execution of self-refining multimodal<br />

consensus clustering on the InternetAds collection are presented. In this case, the<br />

modalities are object (i.e image) attributes and collateral image attributes (see appendix<br />

A.2.2 for a description).<br />

E.2.1 Consensus clustering per modality and across modalities<br />

In this section, the quality of the unimodal, multimodal and intermodal consensus clusterings<br />

obtained on the cluster ensembles generated upon the agglo-cos-upgma, direct-cos-i2,<br />

graph-cos-i2 and rb-cos-i2 clustering algorithms is evaluated.<br />

Firstly, the results corresponding to the agglo-cos-upgma cluster ensemble are depicted<br />

in figure E.9. The first thing to notice is the extremely low quality of the cluster ensemble<br />

components, regardless of the modality. This fact conditions the consensus clustering results<br />

obtained, which are also of very low quality. Moreover, in contrast to what has been observed<br />

in the rest of experiments, there exist very little differences among the performance of the<br />

distinct consensus functions employed.<br />

A very similar behaviour is observed in the experiments conducted on the direct-cos-i2<br />

and rb-cos-i2 cluster ensembles (figures E.10 and E.12). However, pretty different results are<br />

obtained on the graph-cos-i2 cluster ensemble (see figure E.11). In this case, the execution<br />

of consensus clustering on the collateral and the multimodal modalities yields better results.<br />

364<br />

λ 50<br />

c<br />

λ 75<br />

c<br />

λ 30<br />

c<br />

λ 40<br />

c<br />

λ 50<br />

c<br />

λ 75<br />

c

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!