Near Infrared Camera and Multi-Object Spectrometer
E238787
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.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Near Infrared Camera and Multi-Object Spectrometer canonical | 5 |
How this entity was disambiguated
This entity first appeared as the object of triple T2151761 — 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: Near Infrared Camera and Multi-Object Spectrometer Context triple: [STS-82, installedInstrument, Near Infrared Camera and Multi-Object Spectrometer]
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A.
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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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.
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C.
GMOS-S (Gemini Multi-Object Spectrograph South)
GMOS-S (Gemini Multi-Object Spectrograph South) is a versatile optical spectrograph and imager designed for multi-object and long-slit spectroscopy on the Gemini South telescope, enabling detailed studies of faint and distant astronomical sources.
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D.
Mid-Infrared Instrument
The Mid-Infrared Instrument (MIRI) is a key James Webb Space Telescope payload that provides imaging, spectroscopy, and coronagraphy in the mid-infrared range to study cold, distant, and dust-obscured cosmic objects.
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E.
Inamori Magellan Areal Camera and Spectrograph
The Inamori Magellan Areal Camera and Spectrograph (IMACS) is a wide-field optical imaging and spectrographic instrument mounted on the Magellan telescopes, used for deep astronomical surveys and detailed spectroscopic studies.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Near Infrared Camera and Multi-Object Spectrometer Target entity description: 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.
-
A.
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.
-
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.
GMOS-S (Gemini Multi-Object Spectrograph South)
GMOS-S (Gemini Multi-Object Spectrograph South) is a versatile optical spectrograph and imager designed for multi-object and long-slit spectroscopy on the Gemini South telescope, enabling detailed studies of faint and distant astronomical sources.
-
D.
Mid-Infrared Instrument
The Mid-Infrared Instrument (MIRI) is a key James Webb Space Telescope payload that provides imaging, spectroscopy, and coronagraphy in the mid-infrared range to study cold, distant, and dust-obscured cosmic objects.
-
E.
Inamori Magellan Areal Camera and Spectrograph
The Inamori Magellan Areal Camera and Spectrograph (IMACS) is a wide-field optical imaging and spectrographic instrument mounted on the Magellan telescopes, used for deep astronomical surveys and detailed spectroscopic studies.
- F. None of above. chosen
Statements (48)
| Predicate | Object |
|---|---|
| instanceOf |
Hubble Space Telescope instrument
ⓘ
near-infrared camera ⓘ near-infrared spectrometer ⓘ space telescope instrument ⓘ |
| abbreviation | NICMOS ⓘ |
| coolingMethod | cryogenic cooling ⓘ |
| countryOfOrigin |
United States of America
ⓘ
surface form:
United States
|
| deactivatedDate | 1999 ⓘ |
| designedFor |
high-resolution imaging
ⓘ
multi-object spectroscopy ⓘ near-infrared spectroscopy ⓘ studies of distant astronomical objects ⓘ studies of dust-obscured astronomical objects ⓘ studies of faint astronomical objects ⓘ |
| developedBy |
Ball Aerospace
ⓘ
surface form:
Ball Aerospace & Technologies Corp.
University of Arizona ⓘ |
| developedFor |
Hubble Servicing Mission 2
ⓘ
surface form:
Hubble Space Telescope second servicing mission
|
| fieldOfView |
large field camera (Camera 3)
ⓘ
medium field camera (Camera 2) ⓘ small field high-resolution camera (Camera 1) ⓘ |
| finalShutdownDate | 2008 ⓘ |
| firstLightDate | 1997 ⓘ |
| hasCapability |
coronagraphy
ⓘ
imaging ⓘ polarimetry ⓘ spectroscopy ⓘ |
| hasComponent |
Camera 1
ⓘ
Camera 2 ⓘ Camera 3 ⓘ |
| hostObservatory | Low Earth orbit ⓘ |
| installationDate | 1997 ⓘ |
| installedOn |
Hubble Servicing Mission 2
ⓘ
surface form:
Hubble Space Telescope Servicing Mission 2
|
| locatedIn | Hubble Space Telescope axial instrument bay ⓘ |
| operator | NASA ⓘ |
| originalCoolant | solid nitrogen ⓘ |
| reactivatedDate | 2002 ⓘ |
| replacedInstrument | Goddard High Resolution Spectrograph ⓘ |
| scientificGoal |
study of brown dwarfs
ⓘ
study of exoplanetary systems ⓘ study of high-redshift galaxies ⓘ study of protoplanetary disks ⓘ study of star formation in dusty regions ⓘ study of the Galactic center ⓘ |
| spacecraft | Hubble Space Telescope ⓘ |
| spectralCoverage | approximately 0.8 to 2.5 micrometers ⓘ |
| successorInstrument |
Wide Field Camera 3
ⓘ
surface form:
Wide Field Camera 3 infrared channel
|
| usesDetector | HgCdTe array detector ⓘ |
| 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: Near Infrared Camera and Multi-Object Spectrometer Description of subject: 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.
Referenced by (5)
Full triples — surface form annotated when it differs from this entity's canonical label.