Triple
T17661649
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | FMOS |
E440266
|
entity |
| Predicate | acronymFor |
P590
|
FINISHED |
| Object | Fiber Multi-Object Spectrograph |
—
|
NE NERFINISHED |
How this triple was built (2 steps)
Every LLM step that produced this triple, in pipeline order — named-entity classification, the disambiguation choices (the exact options shown, with the pick highlighted), and the generated description. The batch + timestamp of each is in the Provenance table below.
NER
Named-entity recognition
gpt-5-mini
Instruction
Given a phrase, classify it is english named entity (e.g., persons, organizations, works of art) in Latin script, or not (e.g., literals, dates, URLs, verbose phrases). For disambiguation, the statement where the phrase occurs as object is also given. Please return a JSON object with `phrase` (string, the phrase being analyzed) and `is_ne` (boolean, indicating whether the phrase is a Named Entity).
Input
Phrase: Fiber Multi-Object Spectrograph | Statement: [FMOS, acronymFor, Fiber Multi-Object Spectrograph]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Fiber Multi-Object Spectrograph Context triple: [FMOS, acronymFor, Fiber Multi-Object Spectrograph]
-
A.
Fiber Multi-Object Spectrograph
chosen
Fiber Multi-Object Spectrograph is an astronomical instrument designed to simultaneously obtain spectra from many celestial objects using optical fibers.
-
B.
Fiber-fed Extended Range Optical Spectrograph
Fiber-fed Extended Range Optical Spectrograph is a high-resolution echelle spectrograph used in astronomy to obtain precise, wide-wavelength-range stellar spectra, notably for studies such as radial-velocity measurements and stellar characterization.
-
C.
Large Sky Area Multi-Object Fiber Spectroscopic Telescope
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) is a Chinese wide-field optical telescope designed to collect spectra from thousands of celestial objects simultaneously for large-scale sky surveys.
-
D.
Faint Object Spectrograph
The Faint Object Spectrograph was an early-generation Hubble Space Telescope instrument designed to obtain detailed spectra of very dim astronomical objects across a wide range of wavelengths.
-
E.
Infrared Multi-Slit Spectrometer
The Infrared Multi-Slit Spectrometer is a planned TMT instrument designed to obtain simultaneous high-resolution infrared spectra of multiple astronomical targets using a multi-slit configuration.
- F. None of above.
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Provenance (2 batches)
The batch behind each pipeline step, in order, with when it ran. Timestamps are batch-level — stages were processed in waves, so the object chain (NER → NED1 → NEDg → NED2) reads in order, but predicate / elicitation batches can sit in a different wave.
| Step | Stage | Batch ID | Status | When |
|---|---|---|---|---|
| creating | Elicitation | batch_69d8b9e87e18819087104a44dc4dc5b1 |
completed | April 10, 2026, 8:50 a.m. |
| NER | Named-entity recognition | batch_69e46ea67f8081909da164ca21a98675 |
completed | April 19, 2026, 5:56 a.m. |
Created at: April 10, 2026, 9:43 a.m.