5-plex_covering_karate

Source: relF

Source Composite Image

All sources below were be compared against this source composite image.

Instance: 5-plex_covering_karate

Top 49 Most Similar strIPlib Instances

These are the 49 CCM images (for individual instances) that are most similar to the CCM image for this instance, according to the ISS metric.

These are the 49 most similar strIPlib instance CCM images.
Model group: 3-plex_covering_karate Model group: mug88_25.col.disa Model group: d250_21 Model group: d250_13 Model group: R50_1gb.col.bigM Model group: 4-clique_covering_jazz Model group: 0.8-quasi-clique_covering_karate Model group: d250_10 Model group: d250_08_alternative Model group: 0.95-quasi-clique_covering_karate Model group: d750_18 Model group: 0.9-quasi-clique_partitioning_karate Model group: 0.9-quasi-clique_covering_karate Model group: d750_06 Model group: d250_17_alternative Model group: d250_17 Model group: qwhopt.order5.holes10.1.col.bigM Model group: qwhdec.order5.holes10.1.col.bigM Model group: ring_n10p0.1s2 Model group: tr12-30 Model group: 0.95-quasi-clique_partitioning_chesapeake Model group: 0.95-quasi-clique_covering_chesapeake Model group: d750_12 Model group: X11218C Model group: X12117A Model group: X11117E Model group: X12119C Model group: X12418C Model group: X12217E Model group: X12229A Model group: X11427D Model group: qwhdec.order5.holes10.1.col.disa Model group: qwhopt.order5.holes10.1.col.disa Model group: 0.9-quasi-clique_covering_chesapeake Model group: d500_21 Model group: d750_01 Model group: d500_11 Model group: d100_02_alternative Model group: d100_20_alternative Model group: la07 Model group: G53 Model group: n20p5t2s4 Model group: d100_20 Model group: d500_25 Model group: la31 Model group: la34 Model group: d100_11 Model group: la35 Model group: d250_23_alternative Model group: d250_14
Name (Source) 3-plex_covering_karate (relF) mug88_25.col.disa (colD) d250_21 (mapB) d250_13 (mapB) R50_1gb.col.bigM (colG) 4-clique_covering_jazz (relC) 0.8-quasi-clique_covering_karate (relA) d250_10 (mapB) d250_08_alternative (mapA) 0.95-quasi-clique_covering_karate (relA) d750_18 (mapB) 0.9-quasi-clique_partitioning_karate (relB) 0.9-quasi-clique_covering_karate (relA) d750_06 (mapB) d250_17_alternative (mapA) d250_17 (mapB) qwhopt.order5.holes10.1.col.bigM (colA) qwhdec.order5.holes10.1.col.bigM (colA) ring_n10p0.1s2 (pcp) tr12-30 (lotC) 0.95-quasi-clique_partitioning_chesapeake (relB) 0.95-quasi-clique_covering_chesapeake (relA) d750_12 (mapB) X11218C (lotD) X12117A (lotD) X11117E (lotD) X12119C (lotD) X12418C (lotD) X12217E (lotD) X12229A (lotD) X11427D (lotD) qwhdec.order5.holes10.1.col.disa (colB) qwhopt.order5.holes10.1.col.disa (colB) 0.9-quasi-clique_covering_chesapeake (relA) d500_21 (mapB) d750_01 (mapB) d500_11 (mapB) d100_02_alternative (mapA) d100_20_alternative (mapA) la07 (sch) G53 (lotF) n20p5t2s4 (pcp) d100_20 (mapB) d500_25 (mapB) la31 (sch) la34 (sch) d100_11 (mapB) la35 (sch) d250_23_alternative (mapA) d250_14 (mapB)
Rank / ISS The image-based structural similarity (ISS) metric measures the Euclidean distance between two image-based feature vectors. A smaller ISS value indicates greater similarity.
1 / 3.357 2 / 3.649 3 / 3.664 4 / 3.748 5 / 3.800 6 / 3.851 7 / 3.980 8 / 3.990 9 / 4.045 10 / 4.072 11 / 4.074 12 / 4.085 13 / 4.085 14 / 4.097 15 / 4.097 16 / 4.120 17 / 4.122 18 / 4.122 19 / 4.146 20 / 4.157 21 / 4.174 22 / 4.174 23 / 4.181 24 / 4.182 25 / 4.182 26 / 4.182 27 / 4.182 28 / 4.182 29 / 4.182 30 / 4.182 31 / 4.182 32 / 4.186 33 / 4.186 34 / 4.188 35 / 4.188 36 / 4.233 37 / 4.261 38 / 4.262 39 / 4.269 40 / 4.278 41 / 4.282 42 / 4.288 43 / 4.312 44 / 4.313 45 / 4.318 46 / 4.319 47 / 4.336 48 / 4.337 49 / 4.339 50 / 4.349
Updated August 16, 2019