FEROS

E368855

FEROS is a high-resolution echelle spectrograph used on ESO telescopes for precise stellar and exoplanet spectroscopy.

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FEROS canonical 4

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Predicate Object
instanceOf astronomical spectrograph
high-resolution echelle spectrograph
abbreviation FEROS
calibrationSource Thorium-Argon lamp
commissionedBy European Southern Observatory
country Chile
dataArchive ESO Science Archive Facility
dataProduct high-resolution optical spectra
design cross-dispersed echelle
fiber-fed spectrograph
detectorType CCD
environment temperature-controlled room
fullName Fiber-fed Extended Range Optical Spectrograph
hostInstitution MPG/ESO 2.2 m Telescope
surface form: Max Planck Gesellschaft / ESO 2.2-m telescope collaboration
hostTelescopeAperture 1.52 m
2.2 m
installedOn ESO 1.52-metre telescope
MPG/ESO 2.2 m Telescope
surface form: MPG/ESO 2.2-metre telescope
locatedAt La Silla Observatory
mountType Cassegrain focus (via fiber feed)
observatory La Silla Observatory
observingMode high-resolution spectroscopy
simultaneous ThAr calibration (for radial velocities)
operatedBy European Southern Observatory
primaryUse chemical abundance studies
exoplanet spectroscopy
radial velocity measurements
stellar spectroscopy
scienceCase binary star orbits
characterization of exoplanet host stars
search for exoplanets
stellar activity studies
stellar oscillations
site Atacama Desert
surface form: Atacama Desert region of Chile
siteAltitude ~2400 m above sea level
spectralResolution R≈48000
status in operation (as of 2024)
usedFor long-term radial-velocity monitoring programs
measurement of stellar metallicities
measurement of stellar rotational velocities
spectral classification of stars
spectroscopic follow-up of transit candidates
study of emission-line stars
study of evolved stars
study of young stellar objects
wavelengthCoverage 350–920 nm
wavelengthRange optical

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Full triples — surface form annotated when it differs from this entity's canonical label.