Pavo–Indus filament
E511403
The Pavo–Indus filament is a massive, elongated large-scale structure of galaxies forming part of the cosmic web in the nearby universe.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Pavo–Indus filament canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T5336616 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Pavo–Indus filament Context triple: [Hydra–Centaurus Supercluster, contains, Pavo–Indus filament]
-
A.
Shapley Supercluster
The Shapley Supercluster is one of the most massive known concentrations of galaxies in the nearby universe, exerting a significant gravitational influence on surrounding cosmic structures.
-
B.
Hydra–Centaurus Supercluster
The Hydra–Centaurus Supercluster is a massive nearby concentration of galaxy clusters that forms one of the dominant structures in our cosmic neighborhood and serves as a major component of the larger Laniakea Supercluster.
-
C.
Perseus–Pisces Supercluster
The Perseus–Pisces Supercluster is a massive, elongated concentration of galaxy clusters stretching hundreds of millions of light-years across space and forming one of the most prominent large-scale structures in the nearby universe.
-
D.
NGC 6872
NGC 6872 is a highly elongated barred spiral galaxy in the constellation Pavo, notable for being one of the largest known spiral galaxies and for its dramatic tidal interaction with a nearby companion.
-
E.
Virgo Supercluster
The Virgo Supercluster is a massive galaxy supercluster that contains the Local Group, including the Milky Way, and forms part of the larger Laniakea Supercluster.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Pavo–Indus filament Target entity description: The Pavo–Indus filament is a massive, elongated large-scale structure of galaxies forming part of the cosmic web in the nearby universe.
-
A.
Shapley Supercluster
The Shapley Supercluster is one of the most massive known concentrations of galaxies in the nearby universe, exerting a significant gravitational influence on surrounding cosmic structures.
-
B.
Hydra–Centaurus Supercluster
The Hydra–Centaurus Supercluster is a massive nearby concentration of galaxy clusters that forms one of the dominant structures in our cosmic neighborhood and serves as a major component of the larger Laniakea Supercluster.
-
C.
Perseus–Pisces Supercluster
The Perseus–Pisces Supercluster is a massive, elongated concentration of galaxy clusters stretching hundreds of millions of light-years across space and forming one of the most prominent large-scale structures in the nearby universe.
-
D.
NGC 6872
NGC 6872 is a highly elongated barred spiral galaxy in the constellation Pavo, notable for being one of the largest known spiral galaxies and for its dramatic tidal interaction with a nearby companion.
-
E.
Virgo Supercluster
The Virgo Supercluster is a massive galaxy supercluster that contains the Local Group, including the Milky Way, and forms part of the larger Laniakea Supercluster.
- F. None of above. chosen
Statements (29)
| Predicate | Object |
|---|---|
| instanceOf |
galaxy filament
ⓘ
large-scale structure of the universe ⓘ |
| contains |
galaxies
ⓘ
galaxy clusters ⓘ galaxy groups ⓘ |
| hasComponent |
baryonic matter
ⓘ
dark matter ⓘ intergalactic medium ⓘ |
| hasDynamics | influenced by gravity ⓘ |
| hasEnvironment | low-redshift universe ⓘ |
| hasMass | massive ⓘ |
| hasRedshiftRange | low redshift ⓘ |
| hasRole |
connects galaxy clusters
ⓘ
traces matter distribution on large scales ⓘ |
| hasShape | elongated ⓘ |
| hasSignificance |
constrains models of structure formation
ⓘ
traces dark matter distribution ⓘ |
| hasSpatialScale | tens to hundreds of megaparsecs ⓘ |
| hasStructureType | anisotropic ⓘ |
| locatedIn | nearby universe ⓘ |
| namedAfter |
Indus constellation
NERFINISHED
ⓘ
Pavo constellation NERFINISHED ⓘ |
| observedIn |
X-ray wavelengths
ⓘ
optical wavelengths ⓘ radio wavelengths ⓘ |
| partOf | cosmic web ⓘ |
| studiedInField |
extragalactic astronomy
ⓘ
large-scale structure of the cosmos ⓘ observational cosmology ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
Instruction
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Input
Subject: Pavo–Indus filament Description of subject: The Pavo–Indus filament is a massive, elongated large-scale structure of galaxies forming part of the cosmic web in the nearby universe.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.