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neos-3437289-erdre: Instance-to-Instance Comparison Results
Type: | Instance |
Submitter: | Jeff Linderoth |
Description: | (None provided) |
MIPLIB Entry |
Parent Instance (neos-3437289-erdre)
All other instances below were be compared against this "query" instance.![]() ![]() |
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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 | ran14x18-disj-8 [MIPLIB] | neos-848198 [MIPLIB] | neos-933562 [MIPLIB] | neos-5193246-nerang [MIPLIB] | neos-952987 [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 / 0.945 | 2 / 1.004 | 3 / 1.010 | 4 / 1.058 | 5 / 1.062 | |
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 | neos-826650 [MIPLIB] | neos-826224 [MIPLIB] | supportcase14 [MIPLIB] | rococoC11-010100 [MIPLIB] | rococoB10-011000 [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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299 / 1.896 | 614 / 2.106 | 672 / 2.131 | 934 / 2.465 | 955 / 2.569 | |
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 neos-3437289-erdre, the five most similar instances to neos-3437289-erdre according to the MIC, and the five most similar instances to neos-3437289-erdre according to MIPLIB 2017.
INSTANCE | SUBMITTER | DESCRIPTION | ISS | RANK | |
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Parent Instance | neos-3437289-erdre [MIPLIB] | Jeff Linderoth | (None provided) | 0.000000 | - |
MIC Top 5 | ran14x18-disj-8 [MIPLIB] | J. Aronson | Fixed charge transportation problem | 0.945284 | 1 |
neos-848198 [MIPLIB] | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 1.004144 | 2 | |
neos-933562 [MIPLIB] | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 1.010210 | 3 | |
neos-5193246-nerang [MIPLIB] | Jeff Linderoth | (None provided) | 1.058190 | 4 | |
neos-952987 [MIPLIB] | NEOS Server Submission | Instance coming from the NEOS Server with unknown application | 1.062185 | 5 | |
MIPLIB Top 5 | neos-826650 [MIPLIB] | NEOS Server Submission | Instance coming from the NEOS Server with unknown application | 1.896324 | 299 |
neos-826224 [MIPLIB] | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 2.105997 | 614 | |
supportcase14 [MIPLIB] | Michael Winkler | MIP instances collected from Gurobi forum with unknown application | 2.131403 | 672 | |
rococoC11-010100 [MIPLIB] | A. Chabrier, E. Danna, C. Le Pape, L. Perron | Model for dimensioning the arc capacities in a telecommunication network. | 2.464843 | 934 | |
rococoB10-011000 [MIPLIB] | A. Chabrier, E. Danna, C. Le Pape, L. Perron | Model for dimensioning the arc capacities in a telecommunication network | 2.569349 | 955 |
neos-3437289-erdre: Instance-to-Model Comparison Results
Model Group Assignment from MIPLIB: | neos-pseudoapplication-87 |
Assigned Model Group Rank/ISS in the MIC: | 33 / 2.122 |
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 | fhnw-sq | ran | neos-pseudoapplication-22 | neos-pseudoapplication-70 | timtab | |
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 / 1.219 | 2 / 1.459 | 3 / 1.493 | 4 / 1.548 | 5 / 1.694 |
Model Group Summary
The table below contains summary information for the five most similar model groups to neos-3437289-erdre according to the MIC.
MODEL GROUP | SUBMITTER | DESCRIPTION | ISS | RANK | |
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MIC Top 5 | fhnw-sq | Simon Felix | Combinatorial toy fesability problem: Magic square. Models 1 & 2 are feasible, model 3 is unknown. | 1.219211 | 1 |
ran | J. Aronson | Fixed charge transportation problem | 1.458845 | 2 | |
neos-pseudoapplication-22 | Jeff Linderoth | (None provided) | 1.492583 | 3 | |
neos-pseudoapplication-70 | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 1.547690 | 4 | |
timtab | C. Liebchen, R. Möhring | Public transport scheduling problem | 1.693884 | 5 |