HARPS spectrograph

E75065

The HARPS spectrograph is a high-precision, fiber-fed echelle spectrograph designed primarily for detecting exoplanets via radial velocity measurements.

Observed surface forms (3)

Surface form As subject As object
HARPS 0 4
HARPS-N 0 2
High Accuracy Radial velocity Planet Searcher 0 1

Statements (49)

Predicate Object
instanceOf astronomical spectrograph
echelle spectrograph
fiber-fed spectrograph
acronym HARPS spectrograph self-linksurface differs
surface form: HARPS
calibrationMethod simultaneous reference technique
calibrationSource thorium-argon lamp
commissionedIn 2003
countryOfObservatory Chile
dataProduct high-resolution stellar spectra
precise radial velocity time series
designedFor radial velocity measurements
developedBy European Southern Observatory
firstLight 2003
fullName HARPS spectrograph self-linksurface differs
surface form: High Accuracy Radial velocity Planet Searcher
hasUpgrade HARPS spectrograph self-linksurface differs
surface form: HARPS-N
hostObservatory La Silla Observatory
hostTelescopeAperture 3.6 m
inspiredInstrument HARPS spectrograph self-linksurface differs
surface form: HARPS-N
installedOn ESO 3.6 m Telescope
surface form: ESO 3.6 m telescope
isFiberFed yes
isStabilized yes
locatedAt ESO 3.6 m Telescope
surface form: ESO 3.6 m telescope

La Silla Observatory
locatedIn Chile
notableFor high radial-velocity precision for exoplanet searches
observatoryOperator European Southern Observatory
surface form: ESO
observes exoplanet host stars
stars
operatedBy European Southern Observatory
primaryUse exoplanet detection
search for extrasolar planets
radialVelocityPrecision about 1 m/s
sub-meter-per-second
scienceGoals asteroseismology
detection of low-mass exoplanets
measurement of stellar radial velocities
stellar oscillations
study of exoplanetary systems
scientificDiscipline astronomy
astrophysics
exoplanetology
spectralResolution about 115000
stabilityControl temperature control
vacuum enclosure
telescopeType optical telescope
usesEchelleGrating yes
usesOpticalFibers yes
wavelengthCoverage visible
wavelengthRange approximately 380–690 nm

Referenced by (8)

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

HARPS spectrograph acronym HARPS spectrograph self-linksurface differs
this entity surface form: HARPS
HARPS spectrograph fullName HARPS spectrograph self-linksurface differs
this entity surface form: High Accuracy Radial velocity Planet Searcher
La Silla Observatory hasInstrument HARPS spectrograph
ESO 3.6 m Telescope hasSpectrograph HARPS spectrograph
this entity surface form: HARPS
HARPS spectrograph hasUpgrade HARPS spectrograph self-linksurface differs
this entity surface form: HARPS-N
ESO 3.6 m Telescope hostInstrument HARPS spectrograph
this entity surface form: HARPS
HARPS spectrograph inspiredInstrument HARPS spectrograph self-linksurface differs
this entity surface form: HARPS-N
ESO 3.6 m Telescope notableInstrument HARPS spectrograph
this entity surface form: HARPS