Triple
T15838957
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | ACIS |
E384052
|
entity |
| Predicate | fullName |
P16
|
FINISHED |
| Object | Advanced CCD Imaging Spectrometer |
E384051
|
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: Advanced CCD Imaging Spectrometer | Statement: [ACIS, fullName, Advanced CCD Imaging Spectrometer]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Advanced CCD Imaging Spectrometer Context triple: [ACIS, fullName, Advanced CCD Imaging Spectrometer]
-
A.
Advanced CCD Imaging Spectrometer
chosen
The Advanced CCD Imaging Spectrometer is a high-resolution X-ray imaging and spectroscopic camera used on NASA’s Chandra X-ray Observatory to study high-energy astrophysical phenomena.
-
B.
Near Infrared Imager and Slitless Spectrograph
The Near Infrared Imager and Slitless Spectrograph (NIRISS) is a James Webb Space Telescope instrument designed for high-sensitivity near-infrared imaging and spectroscopy, particularly suited for exoplanet characterization and studies of distant galaxies.
-
C.
Near Infrared Camera
The Near Infrared Camera (NIRCam) is a primary imaging instrument on the James Webb Space Telescope designed to capture high-resolution images in the near-infrared spectrum for studying distant galaxies, stars, and exoplanets.
-
D.
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.
-
E.
Space Telescope Imaging Spectrograph
The Space Telescope Imaging Spectrograph is a versatile instrument on the Hubble Space Telescope that performs high-resolution imaging and spectroscopy across ultraviolet, visible, and near-infrared wavelengths to study the physical properties of astronomical objects.
- 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_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. |
Created at: April 10, 2026, 4:49 a.m.