FOcal Reducer and low dispersion Spectrograph 2
E668442
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.
All labels observed (1)
| Label | Occurrences |
|---|---|
| FOcal Reducer and low dispersion Spectrograph 2 canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T7486419 — 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: 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.
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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.
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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.
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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.
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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.
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
Statements (45)
| Predicate | Object |
|---|---|
| instanceOf |
astronomical instrument
ⓘ
focal reducer ⓘ optical spectrograph ⓘ polarimetric instrument ⓘ |
| abbreviation | FORS2 NERFINISHED ⓘ |
| alsoKnownAs | Antu NERFINISHED ⓘ |
| commissionedBy | European Southern Observatory NERFINISHED ⓘ |
| country | Chile ⓘ |
| hasCapability |
imaging polarimetry
ⓘ
long-slit spectroscopy ⓘ multi-object spectroscopy ⓘ spectropolarimetry ⓘ |
| hasComponent |
detector mosaic
ⓘ
filter wheels ⓘ focal reducer optics ⓘ grisms ⓘ |
| hasFeature |
linear polarizers
ⓘ
multi-slit masks ⓘ retarder plates ⓘ wide-field imaging ⓘ |
| hasMode |
imaging mode
ⓘ
polarimetric mode ⓘ spectroscopic mode ⓘ |
| hostTelescope | VLT UT1 Antu NERFINISHED ⓘ |
| locatedIn |
Atacama Desert
ⓘ
Paranal Observatory NERFINISHED ⓘ |
| mountingLocation | Cassegrain focus ⓘ |
| observatory | ESO Very Large Telescope NERFINISHED ⓘ |
| operator | European Southern Observatory NERFINISHED ⓘ |
| organization | ESO NERFINISHED ⓘ |
| partOf | Very Large Telescope NERFINISHED ⓘ |
| scienceUse |
cosmology
ⓘ
extragalactic astronomy ⓘ stellar astronomy ⓘ transient object follow-up ⓘ |
| scientificDomain | astrophysics ⓘ |
| spectralResolution | low ⓘ |
| successorOf | FOcal Reducer and low dispersion Spectrograph NERFINISHED ⓘ |
| telescopeAperture | 8.2-metre class ⓘ |
| telescopeUnit | VLT Unit Telescope 1 NERFINISHED ⓘ |
| usedFor |
imaging
ⓘ
low-resolution spectroscopy ⓘ polarimetry ⓘ |
| usedIn | ground-based optical astronomy ⓘ |
| wavelengthRange | optical ⓘ |
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.
Instruction
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.
Input
Subject: FOcal Reducer and low dispersion Spectrograph 2 Description of subject: 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.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.