HIRES spectrograph

E438728

The HIRES spectrograph is a high-resolution optical spectrograph used on large telescopes to obtain precise stellar and extragalactic spectra for detailed astrophysical studies.

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HIRES spectrograph canonical 1

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Predicate Object
instanceOf astronomical spectrograph
high-resolution echelle spectrograph
optical spectrograph
dataType galaxy spectra
interstellar absorption spectra
quasar spectra
stellar spectra
designedFor precision spectroscopy
enables detailed line-by-line spectral analysis
determination of chemical abundances
determination of stellar radial velocities
measurement of interstellar gas kinematics
measurement of velocity dispersions in galaxies
goal enable detailed astrophysical diagnostics
obtain precise extragalactic spectra
obtain precise stellar spectra
hasCapability high spectral resolving power
multi-order echelle format
precise wavelength calibration
hasSpectralResolution high
measures Doppler shifts of spectral lines
spectral line profiles
wavelength distribution of light
mountedOn large telescopes
observes galaxies
interstellar medium
quasars
stars
operatesIn optical wavelength range
requires large-aperture telescope
scientificDomain astronomy
astrophysics
usedBy professional astronomers
usedFor chemical abundance studies of stars
detailed astrophysical studies
extragalactic spectroscopy
high-resolution spectroscopy
precision radial velocity measurements
quasar absorption line studies
stellar spectroscopy
studies of interstellar medium absorption lines
usedIn high-precision spectroscopic surveys
observational astronomy research

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W. M. Keck Observatory hasInstrument HIRES spectrograph