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neos-3754224-navua: Instance-to-Instance Comparison Results
Type: | Instance |
Submitter: | Jeff Linderoth |
Description: | (None provided) |
MIPLIB Entry |
Parent Instance (neos-3754224-navua)
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 | supportcase23 [MIPLIB] | p500x2988 [MIPLIB] | p500x2988d [MIPLIB] | neos-2075418-temuka [MIPLIB] | 50v-10 [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 / 0.646 | 2 / 0.649 | 3 / 0.671 | 4 / 0.681 | 5 / 0.689 | |
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-619167 [MIPLIB] | neos-5018451-chiese [MIPLIB] | neos-4984115-canche [MIPLIB] | eva1aprime5x5opt [MIPLIB] | eva1aprime6x6opt [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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492 / 1.486 | 587 / 1.581 | 598 / 1.599 | 764 / 1.897 | 803 / 1.990 | |
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-3754224-navua, the five most similar instances to neos-3754224-navua according to the MIC, and the five most similar instances to neos-3754224-navua according to MIPLIB 2017.
INSTANCE | SUBMITTER | DESCRIPTION | ISS | RANK | |
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Parent Instance | neos-3754224-navua [MIPLIB] | Jeff Linderoth | (None provided) | 0.000000 | - |
MIC Top 5 | supportcase23 [MIPLIB] | Michael Winkler | MIP instances collected from Gurobi forum with unknown application | 0.646382 | 1 |
p500x2988 [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 0.648597 | 2 | |
p500x2988d [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 0.671046 | 3 | |
neos-2075418-temuka [MIPLIB] | Hans Mittelmann | Collection of anonymous submissions to the NEOS Server for Optimization | 0.681104 | 4 | |
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. | 0.689382 | 5 | |
MIPLIB Top 5 | neos-619167 [MIPLIB] | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 1.486195 | 492 |
neos-5018451-chiese [MIPLIB] | Jeff Linderoth | (None provided) | 1.581252 | 587 | |
neos-4984115-canche [MIPLIB] | Jeff Linderoth | (None provided) | 1.598858 | 598 | |
eva1aprime5x5opt [MIPLIB] | Yoshihiro Kanno | MILP approach to generate structures with negative thermal expansion coefficients | 1.896880 | 764 | |
eva1aprime6x6opt [MIPLIB] | Yoshihiro Kanno | MILP approach to generate structures with negative thermal expansion coefficients | 1.989988 | 803 |
neos-3754224-navua: Instance-to-Model Comparison Results
Model Group Assignment from MIPLIB: | neos-pseudoapplication-83 |
Assigned Model Group Rank/ISS in the MIC: | 85 / 2.236 |
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 | mc | neos-pseudoapplication-7 | neos-pseudoapplication-99 | noip | pr_product | |
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 / 1.088 | 2 / 1.113 | 3 / 1.116 | 4 / 1.323 | 5 / 1.404 |
Model Group Summary
The table below contains summary information for the five most similar model groups to neos-3754224-navua according to the MIC.
MODEL GROUP | SUBMITTER | DESCRIPTION | ISS | RANK | |
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MIC Top 5 | mc | F. Ortega, L. Wolsey | Fixed cost network flow problems | 1.088057 | 1 |
neos-pseudoapplication-7 | Jeff Linderoth | (None provided) | 1.112909 | 2 | |
neos-pseudoapplication-99 | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 1.116127 | 3 | |
noip | Christopher Hojny | integer programming formulation that verifies that no integer programming formulation of a given 0/1-point set exists | 1.323365 | 4 | |
pr_product | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.403515 | 5 |