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neos-1330346: Instance-to-Instance Comparison Results
Type: | Instance |
Submitter: | NEOS Server Submission |
Description: | Imported from the MIPLIB2010 submissions. |
MIPLIB Entry |
Parent Instance (neos-1330346)
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 | neos-3116779-oban [MIPLIB] | mtest4ma [MIPLIB] | neos-555884 [MIPLIB] | n13-3 [MIPLIB] | n7-3 [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 / 0.434 | 2 / 0.457 | 3 / 0.468 | 4 / 0.469 | 5 / 0.481 | |
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 | acc-tight2 [MIPLIB] | acc-tight4 [MIPLIB] | neos18 [MIPLIB] | acc-tight5 [MIPLIB] | neos-3148108-pahi [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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364 / 1.349 | 712 / 1.838 | 751 / 1.931 | 783 / 1.967 | 835 / 2.145 | |
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-1330346, the five most similar instances to neos-1330346 according to the MIC, and the five most similar instances to neos-1330346 according to MIPLIB 2017.
INSTANCE | SUBMITTER | DESCRIPTION | ISS | RANK | |
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Parent Instance | neos-1330346 [MIPLIB] | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 0.000000 | - |
MIC Top 5 | neos-3116779-oban [MIPLIB] | Jeff Linderoth | (None provided) | 0.434269 | 1 |
mtest4ma [MIPLIB] | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 0.456748 | 2 | |
neos-555884 [MIPLIB] | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 0.468443 | 3 | |
n13-3 [MIPLIB] | A. Atamtürk | Capacitated network design problem | 0.468899 | 4 | |
n7-3 [MIPLIB] | A. Atamtürk | Capacitated network design problem | 0.480955 | 5 | |
MIPLIB Top 5 | acc-tight2 [MIPLIB] | J. Walser | ACC basketball scheduling instance | 1.349195 | 364 |
acc-tight4 [MIPLIB] | J. Walser | ACC basketball scheduling instance | 1.837870 | 712 | |
neos18 [MIPLIB] | NEOS Server Submission | Instance coming from the NEOS Server with unknown application | 1.930732 | 751 | |
acc-tight5 [MIPLIB] | J. Walser | ACC basketball scheduling instance | 1.966857 | 783 | |
neos-3148108-pahi [MIPLIB] | Jeff Linderoth | (None provided) | 2.145240 | 835 |
neos-1330346: Instance-to-Model Comparison Results
Model Group Assignment from MIPLIB: | neos-pseudoapplication-49 |
Assigned Model Group Rank/ISS in the MIC: | 145 / 2.838 |
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 | aflow | noip | neos-pseudoapplication-2 | beasley | neos-pseudoapplication-105 | |
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 / 0.656 | 2 / 0.727 | 3 / 0.755 | 4 / 0.792 | 5 / 0.908 |
Model Group Summary
The table below contains summary information for the five most similar model groups to neos-1330346 according to the MIC.
MODEL GROUP | SUBMITTER | DESCRIPTION | ISS | RANK | |
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MIC Top 5 | aflow | T. Achterberg | Arborescence flow problem on a graph with 40 nodes and edge density 0.9 | 0.655680 | 1 |
noip | Christopher Hojny | integer programming formulation that verifies that no integer programming formulation of a given 0/1-point set exists | 0.726568 | 2 | |
neos-pseudoapplication-2 | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 0.755470 | 3 | |
beasley | F. Ortega, L. Wolsey | Fixed cost network flow problems | 0.792432 | 4 | |
neos-pseudoapplication-105 | Jeff Linderoth | (None provided) | 0.907680 | 5 |