Triple
T4618751
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Milky Way subgroup |
E100928
|
entity |
| Predicate | hasMember |
P10
|
FINISHED |
| Object |
Canis Major Overdensity
The Canis Major Overdensity is a debated stellar overdensity near the plane of the Milky Way, often interpreted as either the remnant core of a disrupted dwarf galaxy or a warp/flare feature of the Galactic disk.
|
E459116
|
NE FINISHED |
Provenance (5 batches)
| Stage | Batch ID | Job type | Status |
|---|---|---|---|
| creating | batch_69bd43cf363c819087fd5ab441b4a3f4 |
elicitation | completed |
| NER | batch_69bd59e247448190ad92f194cb1127c5 |
ner | completed |
| NED1 | batch_69bdfa916f4c8190a53bb37ff46ed0b5 |
ned_source_triple | completed |
| NED2 | batch_69bdff53680c8190a62aace0f0c9f3b3 |
ned_description | completed |
| NEDg | batch_69bdfb5502c48190b7679941b83e6e0c |
nedg | completed |
Created at: March 20, 2026, 1:12 p.m.