Triple
T18734947
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | George R. Ricker |
E458135
|
entity |
| Predicate | notableProject |
P4
|
FINISHED |
| Object | High Energy Transient Explorer (HETE) program |
—
|
NE NERFINISHED |
How this triple was built (3 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: High Energy Transient Explorer (HETE) program | Statement: [George R. Ricker, notableProject, High Energy Transient Explorer (HETE) program]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: High Energy Transient Explorer (HETE) program Context triple: [George R. Ricker, notableProject, High Energy Transient Explorer (HETE) program]
-
A.
High Energy Telescope
The High Energy Telescope is a space-based instrument designed to detect and measure high-energy particles and radiation, contributing to studies of cosmic rays and energetic astrophysical phenomena.
-
B.
Burst Alert Telescope
The Burst Alert Telescope is a high-energy gamma-ray detector on the Neil Gehrels Swift Observatory designed to rapidly locate and trigger follow-up observations of cosmic gamma-ray bursts.
-
C.
Low Energy Telescope
The Low Energy Telescope is a scientific instrument aboard the ACE spacecraft designed to measure the composition and energy spectra of low-energy charged particles in space.
-
D.
Hard X-ray Detector
The Hard X-ray Detector is a space-based instrument designed to observe high-energy X-ray emissions from cosmic sources, enabling studies of phenomena such as black holes, neutron stars, and supernova remnants.
-
E.
High Energy Astronomy Observatory program
The High Energy Astronomy Observatory program was a series of NASA missions in the late 1970s and early 1980s dedicated to studying the universe in high-energy wavelengths such as X-rays and gamma rays.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: High Energy Transient Explorer (HETE) program Target entity description: The High Energy Transient Explorer (HETE) program was a space-based astrophysics mission dedicated to detecting and studying high-energy transient phenomena such as gamma-ray bursts.
-
A.
High Energy Telescope
The High Energy Telescope is a space-based instrument designed to detect and measure high-energy particles and radiation, contributing to studies of cosmic rays and energetic astrophysical phenomena.
-
B.
Burst Alert Telescope
The Burst Alert Telescope is a high-energy gamma-ray detector on the Neil Gehrels Swift Observatory designed to rapidly locate and trigger follow-up observations of cosmic gamma-ray bursts.
-
C.
Low Energy Telescope
The Low Energy Telescope is a scientific instrument aboard the ACE spacecraft designed to measure the composition and energy spectra of low-energy charged particles in space.
-
D.
Hard X-ray Detector
The Hard X-ray Detector is a space-based instrument designed to observe high-energy X-ray emissions from cosmic sources, enabling studies of phenomena such as black holes, neutron stars, and supernova remnants.
-
E.
High Energy Astronomy Observatory program
The High Energy Astronomy Observatory program was a series of NASA missions in the late 1970s and early 1980s dedicated to studying the universe in high-energy wavelengths such as X-rays and gamma rays.
- F. None of above. chosen
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_69d8d393ba9c8190a8b03b04ddbb0a09 |
completed | April 10, 2026, 10:40 a.m. |
| NER | Named-entity recognition | batch_69e56d7ae10081908bc6857d1d147eef |
completed | April 20, 2026, 12:04 a.m. |
Created at: April 10, 2026, 11:51 a.m.