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neos17: Instance-to-Instance Comparison Results
Type: | Instance |
Submitter: | NEOS Server Submission |
Description: | Imported from the MIPLIB2010 submissions. |
MIPLIB Entry |
Parent Instance (neos17)
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 | vpphard [MIPLIB] | vpphard2 [MIPLIB] | neos-4322846-ryton [MIPLIB] | graph40-40-1rand [MIPLIB] | graph40-80-1rand [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 / 0.838 | 2 / 0.840 | 3 / 1.056 | 4 / 1.059 | 5 / 1.064 | |
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-3209519-ruhr [MIPLIB] | neos-3610173-itata [MIPLIB] | neos-3611447-jijia [MIPLIB] | neos-3610040-iskar [MIPLIB] | neos-3611689-kaihu [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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111 / 1.227 | 236 / 1.363 | 305 / 1.437 | 314 / 1.449 | 336 / 1.472 | |
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 neos17, the five most similar instances to neos17 according to the MIC, and the five most similar instances to neos17 according to MIPLIB 2017.
INSTANCE | SUBMITTER | DESCRIPTION | ISS | RANK | |
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Parent Instance | neos17 [MIPLIB] | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 0.000000 | - |
MIC Top 5 | vpphard [MIPLIB] | C. Cardonha | Vehicle positioning problem instance | 0.838082 | 1 |
vpphard2 [MIPLIB] | C. Cardonha | Vehicle positioning problem instance. Solved using CPLEX 12.4 in 43987 seconds (May 2012). Solved using Gurobi 5.6.2 in 124 seconds (May 2014).Solved using CPLEX 12.6 in 225 seconds (May 2014). | 0.839980 | 2 | |
neos-4322846-ryton [MIPLIB] | Jeff Linderoth | (None provided) | 1.056306 | 3 | |
graph40-40-1rand [MIPLIB] | Michael Bastubbe | Packing Cuts in Undirected Graphs. Instances are described in 4.1. | 1.058983 | 4 | |
graph40-80-1rand [MIPLIB] | Michael Bastubbe | Packing Cuts in Undirected Graphs. Instances are described in 4.1. | 1.063810 | 5 | |
MIPLIB Top 5 | neos-3209519-ruhr [MIPLIB] | Jeff Linderoth | (None provided) | 1.227260 | 111 |
neos-3610173-itata [MIPLIB] | Jeff Linderoth | (None provided) | 1.363257 | 236 | |
neos-3611447-jijia [MIPLIB] | Jeff Linderoth | (None provided) | 1.437292 | 305 | |
neos-3610040-iskar [MIPLIB] | Jeff Linderoth | (None provided) | 1.448716 | 314 | |
neos-3611689-kaihu [MIPLIB] | Jeff Linderoth | (None provided) | 1.472438 | 336 |
neos17: Instance-to-Model Comparison Results
Model Group Assignment from MIPLIB: | neos-pseudoapplication-66 |
Assigned Model Group Rank/ISS in the MIC: | 136 / 2.927 |
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 | map | sp_product | rmatr | neos-pseudoapplication-2 | polygonpack | |
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 / 1.294 | 2 / 1.348 | 3 / 1.363 | 4 / 1.366 | 5 / 1.442 |
Model Group Summary
The table below contains summary information for the five most similar model groups to neos17 according to the MIC.
MODEL GROUP | SUBMITTER | DESCRIPTION | ISS | RANK | |
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MIC Top 5 | map | Kiyan Ahmadizadeh | Land parcel selection problems motivated by Red-Cockaded Woodpecker conservation problem | 1.294310 | 1 |
sp_product | MIPLIB submission pool | Imported from the MIPLIB2010 submissions. | 1.348419 | 2 | |
rmatr | Dmitry Krushinsky | Model coming from a formulation of the p-Median problem using square cost matrices | 1.362792 | 3 | |
neos-pseudoapplication-2 | NEOS Server Submission | Imported from the MIPLIB2010 submissions. | 1.366226 | 4 | |
polygonpack | Antonio Frangioni | Given a set P of polygons, not necessarily convex, and a rectangle, we want to find the subset S of P with largest possible total area and a position every p in S so that there are no overlaps and they are all included in the rectangle. We allow a small set of rotations (0, 90, 180, 270 degrees) for every polygon. The problem is simplified w.r.t. the real application because the polygons do not have (fully encircled) "holes", which are supposedly filled-in separately, although they can have "bays". Models are saved as .lp. Model LpPackingModel_Dim means that we are trying to pack polygons taken from set ; there are currently 5 different sets, and is 7, 10 or 15. | 1.441552 | 5 |