Triple
T3549021
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | HARPS spectrograph |
E75065
|
entity |
| Predicate | fullName |
P16
|
FINISHED |
| Object | High Accuracy Radial velocity Planet Searcher |
E75065
|
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: High Accuracy Radial velocity Planet Searcher | Statement: [HARPS spectrograph, fullName, High Accuracy Radial velocity Planet Searcher]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: High Accuracy Radial velocity Planet Searcher Context triple: [HARPS spectrograph, fullName, High Accuracy Radial velocity Planet Searcher]
-
A.
Wide Angle Search for Planets
Wide Angle Search for Planets (WASP) is a ground-based exoplanet survey project that uses wide-field cameras to detect transiting planets around bright stars.
-
B.
WASP exoplanet survey
The WASP exoplanet survey is a ground-based project that uses wide-field telescopes to discover and study transiting exoplanets around bright stars.
-
C.
Doppler spectroscopy
Doppler spectroscopy is a technique that measures frequency shifts in light or other waves to determine the velocity and motion of astronomical objects or particles relative to an observer.
-
D.
NASA Exoplanet Archive
The NASA Exoplanet Archive is an online database and research tool that compiles and provides access to confirmed exoplanet discoveries and related observational data for the scientific community.
-
E.
HARPS spectrograph
chosen
The HARPS spectrograph is a high-precision, fiber-fed echelle spectrograph designed primarily for detecting exoplanets via radial velocity measurements.
- 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_69ad85d33c6c819081d5ac1df13b5680 |
completed | March 8, 2026, 2:21 p.m. |
| NER | Named-entity recognition | batch_69adbfd278348190ad2fa54f4a423541 |
completed | March 8, 2026, 6:28 p.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69b38be9335c81909ba546a079134c8f |
completed | March 13, 2026, 4 a.m. |
Created at: March 8, 2026, 3:20 p.m.