JWST coronagraphy with MIRI
E965902
UNEXPLORED
JWST coronagraphy with MIRI is an observing mode of the James Webb Space Telescope’s Mid-Infrared Instrument that uses specialized masks and optics to block starlight and enable high-contrast imaging of faint structures such as exoplanets and circumstellar disks in the mid-infrared.
All labels observed (1)
| Label | Occurrences |
|---|---|
| JWST coronagraphy with MIRI canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T12175298 — 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.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: JWST coronagraphy with MIRI Context triple: [European MIRI Consortium, contributesTo, JWST coronagraphy with MIRI]
-
A.
Lyot coronagraphs
Lyot coronagraphs are optical devices used in telescopes to block out the bright light of a star so that faint nearby objects, such as exoplanets or circumstellar disks, can be imaged.
-
B.
Metis coronagraph
Metis coronagraph is a specialized telescope instrument designed to block the Sun’s bright disk so it can image and study the faint outer solar corona in visible and ultraviolet light.
-
C.
Coronagraph Instrument
The Coronagraph Instrument is a high-contrast imaging and spectroscopy tool on the Nancy Grace Roman Space Telescope designed to directly observe and characterize exoplanets and faint circumstellar material near bright stars.
-
D.
JWST Integrated Science Instrument Module
The JWST Integrated Science Instrument Module is the central structure on the James Webb Space Telescope that houses and supports its primary science instruments and fine guidance systems.
-
E.
Spectro-Polarimetric High-contrast Exoplanet REsearch
Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) is a high-performance instrument on the Very Large Telescope designed to directly image and characterize exoplanets and circumstellar disks using advanced adaptive optics and polarimetry.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: JWST coronagraphy with MIRI Target entity description: JWST coronagraphy with MIRI is an observing mode of the James Webb Space Telescope’s Mid-Infrared Instrument that uses specialized masks and optics to block starlight and enable high-contrast imaging of faint structures such as exoplanets and circumstellar disks in the mid-infrared.
-
A.
Lyot coronagraphs
Lyot coronagraphs are optical devices used in telescopes to block out the bright light of a star so that faint nearby objects, such as exoplanets or circumstellar disks, can be imaged.
-
B.
Metis coronagraph
Metis coronagraph is a specialized telescope instrument designed to block the Sun’s bright disk so it can image and study the faint outer solar corona in visible and ultraviolet light.
-
C.
Coronagraph Instrument
The Coronagraph Instrument is a high-contrast imaging and spectroscopy tool on the Nancy Grace Roman Space Telescope designed to directly observe and characterize exoplanets and faint circumstellar material near bright stars.
-
D.
JWST Integrated Science Instrument Module
The JWST Integrated Science Instrument Module is the central structure on the James Webb Space Telescope that houses and supports its primary science instruments and fine guidance systems.
-
E.
Spectro-Polarimetric High-contrast Exoplanet REsearch
Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) is a high-performance instrument on the Very Large Telescope designed to directly image and characterize exoplanets and circumstellar disks using advanced adaptive optics and polarimetry.
- F. None of above. chosen
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.