Triple

T15839321
Position Surface form Disambiguated ID Type / Status
Subject BeppoSAX E384060 entity
Predicate primaryInstrument P933 FINISHED
Object Narrow Field Instruments
Narrow Field Instruments were a set of high-resolution, pointed X-ray detectors aboard the BeppoSAX satellite used for detailed observations of cosmic X-ray sources.
E1179675 NE FINISHED

How this triple was built (4 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: Narrow Field Instruments | Statement: [BeppoSAX, primaryInstrument, Narrow Field Instruments]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: Narrow Field Instruments
Context triple: [BeppoSAX, primaryInstrument, Narrow Field Instruments]
  • A. Wide Field Instrument
    The Wide Field Instrument is the primary camera and spectrograph on NASA’s Nancy Grace Roman Space Telescope, designed to capture large-area, high-resolution images for studies of dark energy, exoplanets, and infrared astrophysics.
  • B. Wide Field Optical Spectrometer
    The Wide Field Optical Spectrometer is a planned first-light instrument for the Thirty Meter Telescope designed to capture detailed optical spectra over a large area of the sky for studies of galaxies, stars, and other faint astronomical objects.
  • C. Coudé Echelle Spectrometer
    Coudé Echelle Spectrometer is a high-resolution astronomical spectrograph designed for detailed analysis of stellar and other celestial spectra, typically fed by a telescope’s coudé focus.
  • D. IAC-80 Telescope
    The IAC-80 Telescope is a medium-sized optical telescope used for astronomical research and observations at the Teide Observatory in the Canary Islands.
  • E. NISP instrument
    The NISP instrument is a near-infrared spectrometer and photometer aboard the Euclid space telescope, designed to map the geometry of the dark universe by measuring the shapes and redshifts of distant galaxies.
  • F. None of above. chosen
  • G. Unsure - the case is ambiguous/there is not enough information to decide.
NEDg Description generation gpt-5.1
Instruction
Generate a one-sentence description of the target entity. 
You are given a context triple in the form (subject, predicate, object), where the object is the target entity. 
# Instructions
Use the triple to infer relevant information about the entity. Describe the entity based on what is most defining, well-known. 
Avoid repeating the information from the triple, unless really essential.
# Response Format
Return only the sentence: "Description: [one-sentence description of the target entity]"
Input
Entity: Narrow Field Instruments
Triple: [BeppoSAX, primaryInstrument, Narrow Field Instruments]
Generated description
Narrow Field Instruments were a set of high-resolution, pointed X-ray detectors aboard the BeppoSAX satellite used for detailed observations of cosmic X-ray sources.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: Narrow Field Instruments
Target entity description: Narrow Field Instruments were a set of high-resolution, pointed X-ray detectors aboard the BeppoSAX satellite used for detailed observations of cosmic X-ray sources.
  • A. Wide Field Instrument
    The Wide Field Instrument is the primary camera and spectrograph on NASA’s Nancy Grace Roman Space Telescope, designed to capture large-area, high-resolution images for studies of dark energy, exoplanets, and infrared astrophysics.
  • B. Wide Field Optical Spectrometer
    The Wide Field Optical Spectrometer is a planned first-light instrument for the Thirty Meter Telescope designed to capture detailed optical spectra over a large area of the sky for studies of galaxies, stars, and other faint astronomical objects.
  • C. Coudé Echelle Spectrometer
    Coudé Echelle Spectrometer is a high-resolution astronomical spectrograph designed for detailed analysis of stellar and other celestial spectra, typically fed by a telescope’s coudé focus.
  • D. IAC-80 Telescope
    The IAC-80 Telescope is a medium-sized optical telescope used for astronomical research and observations at the Teide Observatory in the Canary Islands.
  • E. NISP instrument
    The NISP instrument is a near-infrared spectrometer and photometer aboard the Euclid space telescope, designed to map the geometry of the dark universe by measuring the shapes and redshifts of distant galaxies.
  • F. None of above. chosen

Provenance (5 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_69d86da34c888190976e06c4019d415a completed April 10, 2026, 3:25 a.m.
NER Named-entity recognition batch_69e142e4fa24819086a1a226082ac2d3 completed April 16, 2026, 8:13 p.m.
NED1 Entity disambiguation (via context triple) batch_69ffa13c931481908ed9fd10fddd867c completed May 9, 2026, 9:03 p.m.
NEDg Description generation batch_69ffa419c6dc81908c9678f8434530f8 completed May 9, 2026, 9:16 p.m.
NED2 Entity disambiguation (via description) batch_69ffa4cff5088190a7f11fd62941f4fb completed May 9, 2026, 9:19 p.m.
Created at: April 10, 2026, 4:49 a.m.