Triple
T18768584
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Celestron |
E458953
|
entity |
| Predicate | hasNotableTechnology |
P642
|
FINISHED |
| Object |
EdgeHD flat-field optics
EdgeHD flat-field optics is Celestron’s advanced optical design that delivers sharp, coma-free images across a wide, flat field for both visual observing and astrophotography.
|
E1341454
|
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: EdgeHD flat-field optics | Statement: [Celestron, hasNotableTechnology, EdgeHD flat-field optics]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: EdgeHD flat-field optics Context triple: [Celestron, hasNotableTechnology, EdgeHD flat-field optics]
-
A.
Keck II adaptive optics system
The Keck II adaptive optics system is a high-performance real-time wavefront correction facility on the Keck II telescope that sharpens ground-based astronomical images to near space-based resolution.
-
B.
Photodetector Array Camera and Spectrometer
The Photodetector Array Camera and Spectrometer (PACS) was an instrument on the Herschel Space Observatory designed to perform far-infrared imaging and spectroscopy for studying cold dust, gas, and star-forming regions in the universe.
-
C.
Altair adaptive optics system
The Altair adaptive optics system is a high-resolution imaging instrument at the Gemini North telescope that corrects for atmospheric distortion to produce sharper astronomical observations.
-
D.
Advanced CCD Imaging Spectrometer
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.
-
E.
Wide Field Instrument
The Wide Field Instrument is the primary camera and spectrograph on NASA’s Nancy Grace Roman Space Telescope, designed to capture large-area, high-resolution images for studies of dark energy, exoplanets, and infrared astrophysics.
- 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: EdgeHD flat-field optics Triple: [Celestron, hasNotableTechnology, EdgeHD flat-field optics]
Generated description
EdgeHD flat-field optics is Celestron’s advanced optical design that delivers sharp, coma-free images across a wide, flat field for both visual observing and astrophotography.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: EdgeHD flat-field optics Target entity description: EdgeHD flat-field optics is Celestron’s advanced optical design that delivers sharp, coma-free images across a wide, flat field for both visual observing and astrophotography.
-
A.
Keck II adaptive optics system
The Keck II adaptive optics system is a high-performance real-time wavefront correction facility on the Keck II telescope that sharpens ground-based astronomical images to near space-based resolution.
-
B.
Photodetector Array Camera and Spectrometer
The Photodetector Array Camera and Spectrometer (PACS) was an instrument on the Herschel Space Observatory designed to perform far-infrared imaging and spectroscopy for studying cold dust, gas, and star-forming regions in the universe.
-
C.
Altair adaptive optics system
The Altair adaptive optics system is a high-resolution imaging instrument at the Gemini North telescope that corrects for atmospheric distortion to produce sharper astronomical observations.
-
D.
Advanced CCD Imaging Spectrometer
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.
-
E.
Wide Field Instrument
The Wide Field Instrument is the primary camera and spectrograph on NASA’s Nancy Grace Roman Space Telescope, designed to capture large-area, high-resolution images for studies of dark energy, exoplanets, and infrared astrophysics.
- 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_69d8d395dba0819087568404508590cb |
completed | April 10, 2026, 10:40 a.m. |
| NER | Named-entity recognition | batch_69e58d867264819098ae35c9feab3bb4 |
completed | April 20, 2026, 2:20 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a053d450c8081908e44744a63e15fc3 |
completed | May 14, 2026, 3:11 a.m. |
| NEDg | Description generation | batch_6a053e7376ec8190950881d90d9fa567 |
completed | May 14, 2026, 3:16 a.m. |
| NED2 | Entity disambiguation (via description) | batch_6a053ef3600881908e39a4abe4e032e8 |
completed | May 14, 2026, 3:18 a.m. |
Created at: April 10, 2026, 11:52 a.m.