Triple

T7486419
Position Surface form Disambiguated ID Type / Status
Subject FORS2 E176892 entity
Predicate fullName P16 FINISHED
Object FOcal Reducer and low dispersion Spectrograph 2
FOcal Reducer and low dispersion Spectrograph 2 (FORS2) is a versatile optical instrument on ESO’s Very Large Telescope used for imaging, polarimetry, and low-resolution spectroscopy of astronomical objects.
E668442 NE FINISHED

How this triple was built (4 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: FOcal Reducer and low dispersion Spectrograph 2 | Statement: [FORS2, fullName, FOcal Reducer and low dispersion Spectrograph 2]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: FOcal Reducer and low dispersion Spectrograph 2
Context triple: [FORS2, fullName, FOcal Reducer and low dispersion Spectrograph 2]
  • A. Faint Object Spectrograph
    The Faint Object Spectrograph was an early-generation Hubble Space Telescope instrument designed to obtain detailed spectra of very dim astronomical objects across a wide range of wavelengths.
  • B. Low Dispersion Survey Spectrograph 3
    Low Dispersion Survey Spectrograph 3 is an astronomical instrument used on large telescopes to obtain low-resolution spectra of many celestial objects simultaneously for survey and follow-up observations.
  • C. Fiber-fed Extended Range Optical Spectrograph
    Fiber-fed Extended Range Optical Spectrograph is a high-resolution echelle spectrograph used in astronomy to obtain precise, wide-wavelength-range stellar spectra, notably for studies such as radial-velocity measurements and stellar characterization.
  • D. Boller and Chivens spectrograph
    The Boller and Chivens spectrograph is an astronomical instrument designed for dispersing and analyzing light from celestial objects to study their physical and chemical properties.
  • E. DEIMOS spectrograph
    The DEIMOS spectrograph is a powerful multi-object optical spectrograph designed for wide-field, high-resolution spectroscopy of faint astronomical sources.
  • 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: FOcal Reducer and low dispersion Spectrograph 2
Triple: [FORS2, fullName, FOcal Reducer and low dispersion Spectrograph 2]
Generated description
FOcal Reducer and low dispersion Spectrograph 2 (FORS2) is a versatile optical instrument on ESO’s Very Large Telescope used for imaging, polarimetry, and low-resolution spectroscopy of astronomical objects.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07
Target entity: FOcal Reducer and low dispersion Spectrograph 2
Target entity description: FOcal Reducer and low dispersion Spectrograph 2 (FORS2) is a versatile optical instrument on ESO’s Very Large Telescope used for imaging, polarimetry, and low-resolution spectroscopy of astronomical objects.
  • A. Faint Object Spectrograph
    The Faint Object Spectrograph was an early-generation Hubble Space Telescope instrument designed to obtain detailed spectra of very dim astronomical objects across a wide range of wavelengths.
  • B. Low Dispersion Survey Spectrograph 3
    Low Dispersion Survey Spectrograph 3 is an astronomical instrument used on large telescopes to obtain low-resolution spectra of many celestial objects simultaneously for survey and follow-up observations.
  • C. Fiber-fed Extended Range Optical Spectrograph
    Fiber-fed Extended Range Optical Spectrograph is a high-resolution echelle spectrograph used in astronomy to obtain precise, wide-wavelength-range stellar spectra, notably for studies such as radial-velocity measurements and stellar characterization.
  • D. Boller and Chivens spectrograph
    The Boller and Chivens spectrograph is an astronomical instrument designed for dispersing and analyzing light from celestial objects to study their physical and chemical properties.
  • E. DEIMOS spectrograph
    The DEIMOS spectrograph is a powerful multi-object optical spectrograph designed for wide-field, high-resolution spectroscopy of faint astronomical sources.
  • F. None of above. chosen

Provenance (5 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_69c69f24ac508190bb98fe927c0bd065 completed March 27, 2026, 3:15 p.m.
NER Named-entity recognition batch_69c6f556955c8190bf014a065e04c5d8 completed March 27, 2026, 9:23 p.m.
NED1 Entity disambiguation (via context triple) batch_69c83c68bcf081908a2c280152d887f0 completed March 28, 2026, 8:39 p.m.
NEDg Description generation batch_69c83ddda5688190be1ec69f23671f60 completed March 28, 2026, 8:45 p.m.
NED2 Entity disambiguation (via description) batch_69c83e42b0048190b1abd8ae99c97e38 completed March 28, 2026, 8:46 p.m.
Created at: March 27, 2026, 3:42 p.m.