Triple
T9808986
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | IR G102 grism |
E238220
|
entity |
| Predicate | observingMode |
P8700
|
FINISHED |
| Object | WFC3/IR G102 grism mode |
E238220
|
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: WFC3/IR G102 grism mode | Statement: [IR G102 grism, observingMode, WFC3/IR G102 grism mode]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: WFC3/IR G102 grism mode Context triple: [IR G102 grism, observingMode, WFC3/IR G102 grism mode]
-
A.
IR G102 grism
chosen
The IR G102 grism is an infrared dispersive element on the Hubble Space Telescope’s Wide Field Camera 3 used for low-resolution slitless spectroscopy over near-infrared wavelengths.
-
B.
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.
-
C.
Cosmic Origins Spectrograph
The Cosmic Origins Spectrograph is a highly sensitive ultraviolet spectrograph on the Hubble Space Telescope designed to study the origins and evolution of galaxies, stars, and the intergalactic medium.
-
D.
IFS – Integral Field Spectrograph
IFS – Integral Field Spectrograph is an instrument within the SPHERE exoplanet imaging system on the Very Large Telescope that provides spatially resolved spectroscopy to study exoplanets and circumstellar environments.
-
E.
OSIRIS spectrograph
The OSIRIS spectrograph is a near-infrared integral field spectrograph and imager used on large telescopes to obtain detailed spatial and spectral information from 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_69ca84defac48190abc1148804f184c1 |
completed | March 30, 2026, 2:12 p.m. |
| NER | Named-entity recognition | batch_69cdb21ef32c8190ab4b09d157798451 |
completed | April 2, 2026, 12:02 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_69d1cc5b4dd8819088c86946b4eb8a39 |
completed | April 5, 2026, 2:43 a.m. |
Created at: March 30, 2026, 8:29 p.m.