The echelle more commonly known as the "ladder" or "rack" was a long table that the accused would lie upon and be stretched violently.

The primary instrument attached to the telescope was a fiber-fed, cross-dispersed echelle spectrograph.

The development of echelle spectrometers allowed high-resolution spectroscopy with a much more compact instrument, one which can sometimes be successfully mounted on the Cassegrain focus.

Diffraction-limited imaging and echelle spectroscopy (resolving power 50,000) at mid-infrared wavelengths (8-28 μm)

Nouvelle Echelle métrique de l'Intelligence (in two volumes in collaboration with other authors, 1966)

HARPS is a fibre-fed high resolution echelle spectrograph dedicated to the discovery of extrasolar planets.

Vue de Hounkiar-Iskelesi, Echelle du Grand-Seigneur.

It is use for astronomy, and runs the CORALIE echelle spectrograph to search for planets.

Interview with Henry S. Fitch, conducted on September 6, 1998 by his daughter Alice Fitch Echelle and her family.

The most common monochromator is the Czerny-Turner type whilst the most common polychromator is the Echelle type.

Is a survey of start searching for planets using the MIKE echelle spectrograph mounted on the 6.5m Magellan II (Clay) telescope.

Threatened fishes of the world:Cyprinidon pecosensis (Echelle & Echelle 1978)(Cyprinodontae).

UVES (Ultraviolet and Visual Echelle Spectrograph) is an ultraviolet and visible light spectrograph.

TRIPPEL is a Littrow spectrograph using a 79 grooves/mm echelle grating with a blaze angle of 63.43 degrees.

Potsdam Echelle Polarimetric & Spectroscopic Instrument (PEPSI)

During this study, 13 Doppler measurements of the star were done over a 6 month period using the High Resolution Echelle Spectrometer (HIRES).

Evidence for a planetary companion to HD 100546 was gathered using the UVES echelle spectrograph at the VLT in Chile.

The former uncorrected time scale continues to be published, under the name EAL (Echelle Atomique Libre, meaning Free Atomic Scale).

Follow-up observations by the High Resolution Echelle Spectrometer at Hawaii's W.M. Keck Observatory yielded additional information about the planet, including its mass and radius.

Observations are made using the AAT and the University College London Echelle Spectrograph or UCLES.

The star was studied through the Magellan Inamori Kyocera Echelle spectrograph's (MIKE) ability to use Doppler spectroscopy to measure radial velocity.

Use of the FIES echelle spectrograph at the Nordic Optical Telescope in the Canary Islands gained other spectral measurements that yielded the characteristics of the star.

HIRES, a high resolution echelle spectrometer for the Keck ten-meter telescope: phase C, HIRES core - Issue 57 of Lick Observatory technical reports.

The Fibre-Fed Echelle Spectrograph on the Nordic Optical Telescope gathered additional measurements of WASP-13's spectrum, allowing astronomers to determine WASP-13's characteristics.

Between August 2007 and December 2010, twenty-eight spectra were collected using the High Resolution Echelle Spectrometer (HIRES) at the W.M. Keck Observatory in Hawaii.