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.