Triple
T1000503
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Canis Major Dwarf Galaxy |
E21591
|
entity |
| Predicate | alternativeName |
P39
|
FINISHED |
| Object |
CMa Overdensity
CMa Overdensity is a debated stellar overdensity in the direction of Canis Major, thought by some astronomers to be the remnant of a disrupted dwarf galaxy merging with the Milky Way.
|
E118797
|
NE FINISHED |
Provenance (5 batches)
| Stage | Batch ID | Job type | Status |
|---|---|---|---|
| creating | batch_69a493c476b48190b41fc5e793171cc6 |
elicitation | completed |
| NER | batch_69a4b4fb18b88190ae2d620aaaff4f90 |
ner | completed |
| NED1 | batch_69ac2a1cb4f08190b1351aadd57c3bda |
ned_source_triple | completed |
| NED2 | batch_69ac2bb03508819095f791903f048351 |
ned_description | completed |
| NEDg | batch_69ac2b0d1b348190b4a34bf1c9b43968 |
nedg | completed |
Created at: March 1, 2026, 7:41 p.m.