Triple

T15839801
Position Surface form Disambiguated ID Type / Status
Subject HEASoft E384071 entity
Predicate includesComponent P1393 FINISHED
Object FTOOLS E384072 NE FINISHED

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: FTOOLS | Statement: [HEASoft, includesComponent, FTOOLS]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: FTOOLS
Context triple: [HEASoft, includesComponent, FTOOLS]
  • A. FTOOLS chosen
    FTOOLS is a widely used software package that provides a suite of utilities for analyzing and processing high-energy astrophysics data from space- and ground-based observatories.
  • B. HEASoft software suite
    HEASoft software suite is a collection of data analysis tools widely used in high-energy astrophysics for processing and interpreting X-ray and gamma-ray observations from space- and ground-based missions.
  • C. FOCAL
    FOCAL is an early interactive programming language developed by Digital Equipment Corporation, commonly used on PDP-series minicomputers for scientific and educational purposes.
  • D. VST telescope
    The VST telescope is a 2.6-meter wide-field survey telescope at ESO’s Paranal Observatory in Chile, designed primarily for large-scale imaging of the southern sky in visible light.
  • E. Wide Field Optical Spectrometer (WFOS)
    The Wide Field Optical Spectrometer (WFOS) is a planned wide-field, multi-object optical spectrograph designed to provide high-throughput spectroscopy for large samples of astronomical targets on the Thirty Meter Telescope.
  • F. None of above.
  • G. Unsure - the case is ambiguous/there is not enough information to decide.

Provenance (3 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_69e142e69360819091ea0556bd66d785 completed April 16, 2026, 8:13 p.m.
NED1 Entity disambiguation (via context triple) batch_69ffa13c931481908ed9fd10fddd867c completed May 9, 2026, 9:03 p.m.
Created at: April 10, 2026, 4:49 a.m.