Triple
T9808990
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | IR G102 grism |
E238220
|
entity |
| Predicate | complementaryTo |
P162
|
FINISHED |
| Object |
WFC3 IR G141 grism
The WFC3 IR G141 grism is a near-infrared slitless spectroscopic element on the Hubble Space Telescope’s Wide Field Camera 3, used to obtain low-resolution spectra of astronomical sources over a broad wavelength range.
|
E238220
|
NE FINISHED |
How this triple was built (5 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 G141 grism | Statement: [IR G102 grism, complementaryTo, WFC3 IR G141 grism]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: WFC3 IR G141 grism Context triple: [IR G102 grism, complementaryTo, WFC3 IR G141 grism]
-
A.
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.
-
B.
NIRSpec
NIRSpec is a powerful near-infrared spectrograph on the James Webb Space Telescope designed to analyze the light from distant astronomical objects to study their composition, motion, and physical properties.
-
C.
NIRCam
NIRCam is the primary near-infrared imaging camera on the James Webb Space Telescope, designed for high-resolution observations of distant galaxies, stars, and exoplanets.
-
D.
IR G102 grism
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.
-
E.
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.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NEDg
Description generation
gpt-5.1
Instruction
Generate a one-sentence description of the target entity. You are given a context triple in the form (subject, predicate, object), where the object is the target entity. # Instructions Use the triple to infer relevant information about the entity. Describe the entity based on what is most defining, well-known. Avoid repeating the information from the triple, unless really essential. # Response Format Return only the sentence: "Description: [one-sentence description of the target entity]"
Input
Entity: WFC3 IR G141 grism Triple: [IR G102 grism, complementaryTo, WFC3 IR G141 grism]
Generated description
The WFC3 IR G141 grism is a near-infrared slitless spectroscopic element on the Hubble Space Telescope’s Wide Field Camera 3, used to obtain low-resolution spectra of astronomical sources over a broad wavelength range.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: WFC3 IR G141 grism Target entity description: The WFC3 IR G141 grism is a near-infrared slitless spectroscopic element on the Hubble Space Telescope’s Wide Field Camera 3, used to obtain low-resolution spectra of astronomical sources over a broad wavelength range.
-
A.
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.
-
B.
NIRSpec
NIRSpec is a powerful near-infrared spectrograph on the James Webb Space Telescope designed to analyze the light from distant astronomical objects to study their composition, motion, and physical properties.
-
C.
NIRCam
NIRCam is the primary near-infrared imaging camera on the James Webb Space Telescope, designed for high-resolution observations of distant galaxies, stars, and exoplanets.
-
D.
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.
-
E.
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.
- F. None of above.
PD
Predicate disambiguation
gpt-5-mini-2025-08-07
Target predicate: complementaryTo Context triple: [IR G102 grism, complementaryTo, WFC3 IR G141 grism]
-
A.
complement
Indicates that one entity completes, enhances, or makes another entity whole or more effective by providing what it lacks.
-
B.
complements
chosen
Indicates that one entity enhances, completes, or improves another by providing qualities or functions that fit well together.
-
C.
relatesComplementTo
Indicates that one entity serves as a complement or completing counterpart to another entity within a specified context or structure.
-
D.
requiresComplement
Indicates that one entity depends on another entity as a necessary complement to be complete, functional, or valid.
-
E.
laterComplementedBy
Indicates that an earlier entity is subsequently supplemented, enhanced, or completed by a later entity.
- F. None of above.
Provenance (6 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. |
| NEDg | Description generation | batch_69d1cd7f41448190b387109235dbc7f5 |
completed | April 5, 2026, 2:48 a.m. |
| NED2 | Entity disambiguation (via description) | batch_69d1cdefca5c8190a673caca42aaa7d0 |
completed | April 5, 2026, 2:50 a.m. |
| PD | Predicate disambiguation | batch_69cd03dd2da881909052fbf29736a773 |
completed | April 1, 2026, 11:39 a.m. |
Created at: March 30, 2026, 8:29 p.m.