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fiber: Instance-to-Instance Comparison Results
Type: | Instance |
Submitter: | MIPLIB submission pool |
Description: | Imported from the MIPLIB2010 submissions. |
MIPLIB Entry |
Parent Instance (fiber)
All other instances below were be compared against this "query" instance.
Raw
This is the CCM image before the decomposition procedure has been applied.
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Decomposed
This is the CCM image after a decomposition procedure has been applied. This is the image used by the MIC's image-based comparisons for this query instance.
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Composite of MIC Top 5
Composite of the five decomposed CCM images from the MIC Top 5.
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Composite of MIPLIB Top 5
Composite of the five decomposed CCM images from the MIPLIB Top 5.
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Model Group Composite Image
Composite of the decomposed CCM images for every instance in the same model group as this query.
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MIC Top 5 Instances
These are the 5 decomposed CCM images that are most similar to decomposed CCM image for the the query instance, according to the ISS metric.
Decomposed
These decomposed images were created by GCG.
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Name | neos-3068746-nene [MIPLIB] | dcmulti [MIPLIB] | opt1217 [MIPLIB] | 50v-10 [MIPLIB] | gt2 [MIPLIB] | |
Rank / ISS
The image-based structural similarity (ISS) metric measures the Euclidean distance between the image-based feature vectors for the query instance and all other instances. A smaller ISS value indicates greater similarity.
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1 / 1.005 | 2 / 1.037 | 3 / 1.081 | 4 / 1.083 | 5 / 1.108 | |
Raw
These images represent the CCM images in their raw forms (before any decomposition was applied) for the MIC top 5.
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MIPLIB Top 5 Instances
These are the 5 instances that are most closely related to the query instance, according to the instance statistic-based similarity measure employed by MIPLIB 2017
Decomposed
These decomposed images were created by GCG.
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Name | nu120-pr12 [MIPLIB] | rococoC11-010100 [MIPLIB] | neos-826650 [MIPLIB] | nu25-pr12* [MIPLIB] | nu120-pr9* [MIPLIB] | |
Rank / ISS
The image-based structural similarity (ISS) metric measures the Euclidean distance between the image-based feature vectors for the query instance and all model groups. A smaller ISS value indicates greater similarity.
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408 / 1.553 | 689 / 1.794 | 820 / 2.051 | 408* / 1.553* | 386* / 1.534* | |
Raw
These images represent the CCM images in their raw forms (before any decomposition was applied) for the MIPLIB top 5.
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Instance Summary
The table below contains summary information for fiber, the five most similar instances to fiber according to the MIC, and the five most similar instances to fiber according to MIPLIB 2017.
INSTANCE | SUBMITTER | DESCRIPTION | ISS | RANK | |
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Parent Instance | fiber [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 0.000000 | - |
MIC Top 5 | neos-3068746-nene [MIPLIB] | Jeff Linderoth | (None provided) | 1.005052 | 1 |
dcmulti [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.036656 | 2 | |
opt1217 [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.081454 | 3 | |
50v-10 [MIPLIB] | Serge Bisaillon | Network loading instance. Solved using ug[SCIP/spx], a distributed massively parallel version of SCIP run on 2,000 cores at the HLRN-II super computer facility. | 1.083100 | 4 | |
gt2 [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.107764 | 5 | |
MIPLIB Top 5 | nu120-pr12 [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.553465 | 408 |
rococoC11-010100 [MIPLIB] | A. Chabrier, E. Danna, C. Le Pape, L. Perron | Model for dimensioning the arc capacities in a telecommunication network. | 1.794475 | 689 | |
neos-826650 [MIPLIB] | NEOS Server Submission | Instance coming from the NEOS Server with unknown application | 2.051323 | 820 | |
nu25-pr12* [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.553465* | 408* | |
nu120-pr9* [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.534206* | 386* |
fiber: Instance-to-Model Comparison Results
Model Group Assignment from MIPLIB: | no model group assignment |
Assigned Model Group Rank/ISS in the MIC: | N.A. / N.A. |
MIC Top 5 Model Groups
These are the 5 model group composite (MGC) images that are most similar to the decomposed CCM image for the query instance, according to the ISS metric.
These are model group composite (MGC) images for the MIC top 5 model groups.
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Name | neos-pseudoapplication-74 | scp | mc | oocsp-racks | neos-pseudoapplication-109 | |
Rank / ISS
The image-based structural similarity (ISS) metric measures the Euclidean distance between the image-based feature vectors for the query instance and all other instances. A smaller ISS value indicates greater similarity.
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1 / 1.527 | 2 / 1.674 | 3 / 1.747 | 4 / 1.750 | 5 / 1.755 |
Model Group Summary
The table below contains summary information for the five most similar model groups to fiber according to the MIC.
MODEL GROUP | SUBMITTER | DESCRIPTION | ISS | RANK | |
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MIC Top 5 | neos-pseudoapplication-74 | Jeff Linderoth | (None provided) | 1.526977 | 1 |
scp | Shunji Umetani | This is a random test model generator for SCP using the scheme of the following paper, namely the column cost c[j] are integer randomly generated from [1,100]; every column covers at least one row; and every row is covered by at least two columns. see reference: E. Balas and A. Ho, Set covering algorithms using cutting planes, heuristics, and subgradient optimization: A computational study, Mathematical Programming, 12 (1980), 37-60. We have newly generated Classes I-N with the following parameter values, where each class has five models. We have also generated reduced models by a standard pricing method in the following paper: S. Umetani and M. Yagiura, Relaxation heuristics for the set covering problem, Journal of the Operations Research Society of Japan, 50 (2007), 350-375. You can obtain the model generator program from the following web site. https://sites.google.com/site/shunjiumetani/benchmark | 1.673746 | 2 | |
mc | F. Ortega, L. Wolsey | Fixed cost network flow problems | 1.747406 | 3 | |
oocsp-racks | Gleb Belov | These are the models from MiniZinc Challenges 2012-2016 (see www.minizinc.org), compiled for MIP WITH INDICATOR CONSTRAINTS using the develop branch of MiniZinc and CPLEX 12.7.1 on 30 April 2017. Thus, these models can only be handled by solvers accepting indicator constraints. For models compiled with big-M/domain decomposition only, see my previous submission to MIPLIB.To recompile, create a directory MODELS, a list lst12_16.txt of the models with full paths to mzn/dzn files of each model per line, and say$> ~/install/libmzn/tests/benchmarking/mzn-test.py -l ../lst12_16.txt -slvPrf MZN-CPLEX -debug 1 -addOption "-timeout 3 -D fIndConstr=true -D fMIPdomains=false" -useJoinedName "-writeModel MODELS_IND/%s.mps" Alternatively, you can compile individual model as follows: $> mzn-cplex -v -s -G linear -output-time ../challenge_2012_2016/mznc2016_probs/zephyrus/zephyrus.mzn ../challenge_2012_2016/mznc2016_p/zephyrus/14__8__6__3.dzn -a -timeout 3 -D fIndConstr=true -D fMIPdomains=false -writeModel MODELS_IND/challenge_2012_2016mznc2016_probszephyruszephyrusmzn-challenge_2012_2016mznc2016_probszephyrus14__8__6__3dzn.mps | 1.750473 | 4 | |
neos-pseudoapplication-109 | Jeff Linderoth | (None provided) | 1.755393 | 5 |