FLoridA Multi-object Imaging Near-Infrared Grism Observational Spectrometer 2
E409012
FLAMINGOS-2 is a near-infrared imaging and multi-object spectrograph instrument used on large telescopes for wide-field astronomical observations.
All labels observed (2)
How this entity was disambiguated
This entity first appeared as the object of triple T4031929 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: FLoridA Multi-object Imaging Near-Infrared Grism Observational Spectrometer 2 Context triple: [FLAMINGOS-2, fullName, FLoridA Multi-object Imaging Near-Infrared Grism Observational Spectrometer 2]
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A.
Near Infrared Camera and Multi-Object Spectrometer
The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a Hubble Space Telescope instrument designed to capture high-resolution images and spectra in the near-infrared, enabling studies of faint, distant, and dust-obscured astronomical objects.
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B.
NIFS (Near-Infrared Integral Field Spectrometer)
NIFS (Near-Infrared Integral Field Spectrometer) is an astronomical instrument that provides three-dimensional near-infrared spectroscopy, enabling detailed spatial and spectral studies of celestial objects.
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C.
Near Infrared Imager and Slitless Spectrograph
The Near Infrared Imager and Slitless Spectrograph (NIRISS) is a James Webb Space Telescope instrument designed for high-sensitivity near-infrared imaging and spectroscopy, particularly suited for exoplanet characterization and studies of distant galaxies.
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D.
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.
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E.
MMIRS (Magellan/MMT Infrared Spectrograph)
MMIRS (Magellan/MMT Infrared Spectrograph) is a near-infrared imaging spectrograph designed for the Magellan and MMT telescopes to study faint astronomical objects at infrared wavelengths.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: FLoridA Multi-object Imaging Near-Infrared Grism Observational Spectrometer 2 Target entity description: FLAMINGOS-2 is a near-infrared imaging and multi-object spectrograph instrument used on large telescopes for wide-field astronomical observations.
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A.
Near Infrared Camera and Multi-Object Spectrometer
The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a Hubble Space Telescope instrument designed to capture high-resolution images and spectra in the near-infrared, enabling studies of faint, distant, and dust-obscured astronomical objects.
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B.
NIFS (Near-Infrared Integral Field Spectrometer)
NIFS (Near-Infrared Integral Field Spectrometer) is an astronomical instrument that provides three-dimensional near-infrared spectroscopy, enabling detailed spatial and spectral studies of celestial objects.
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C.
Near Infrared Imager and Slitless Spectrograph
The Near Infrared Imager and Slitless Spectrograph (NIRISS) is a James Webb Space Telescope instrument designed for high-sensitivity near-infrared imaging and spectroscopy, particularly suited for exoplanet characterization and studies of distant galaxies.
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D.
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.
-
E.
MMIRS (Magellan/MMT Infrared Spectrograph)
MMIRS (Magellan/MMT Infrared Spectrograph) is a near-infrared imaging spectrograph designed for the Magellan and MMT telescopes to study faint astronomical objects at infrared wavelengths.
- F. None of above. chosen
Statements (36)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical instrument
ⓘ
multi-object spectrograph ⓘ near-infrared imager ⓘ |
| acronym | FLAMINGOS-2 ⓘ |
| capability |
long-slit spectroscopy
ⓘ
multi-object spectroscopy ⓘ wide-field imaging ⓘ |
| dataProduct |
near-infrared images
ⓘ
near-infrared spectra ⓘ |
| designedFor |
faint object observations
ⓘ
survey science ⓘ |
| electromagneticBand |
infrared
ⓘ
near-infrared ⓘ |
| fieldOfView | wide field ⓘ |
| fullName | FLoridA Multi-object Imaging Near-Infrared Grism Observational Spectrometer 2 self-linksurface differs ⓘ |
| hasComponent |
grism
ⓘ
imaging camera ⓘ multi-object slit masks ⓘ |
| observes |
Galactic objects
ⓘ
astronomical sources ⓘ extragalactic objects ⓘ |
| operationalMode |
imaging mode
ⓘ
spectroscopic mode ⓘ |
| predecessor | FLAMINGOS ⓘ |
| scientificDomain |
astronomy
ⓘ
astrophysics ⓘ |
| spectralRegion |
H band
ⓘ
J band ⓘ K band ⓘ |
| technique |
grism spectroscopy
ⓘ
multi-object spectroscopy ⓘ |
| usedFor |
near-infrared surveys
ⓘ
spectroscopic follow-up ⓘ wide-field astronomical observations ⓘ |
| usedOn | large telescopes ⓘ |
| wavelengthRange | near-infrared ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Subject: FLoridA Multi-object Imaging Near-Infrared Grism Observational Spectrometer 2 Description of subject: FLAMINGOS-2 is a near-infrared imaging and multi-object spectrograph instrument used on large telescopes for wide-field astronomical observations.
Referenced by (5)
Full triples — surface form annotated when it differs from this entity's canonical label.