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.