「spectrograph」の共起表現一覧(1語右で並び替え)

spectrograph

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  • a ray spectrometer, a near-infrared imaging spectrograph, a multi-spectral camera fitted with a CCD
  • l Investigator for the Ultra-Violet Imaging Spectrograph aboard the NASA Cassini-Huygens unmanned mi
  • es under Howell using a new Rowland grating spectrograph acquired by Smith College to research the e
  • in their success was the development of the spectrograph, an instrument which replaced several wet c
  • With Louis G. Henyey he invented a new spectrograph and a wide-field camera.
  • users, while Gecko, a very high resolution spectrograph, and MOS, the Multi Object Spectrograph, ca
  • Image taken by ESO Faint Object Spectrograph and Camera attached to the 3.6-metre telesc
  • class telescope, a high dispersion echelle spectrograph, and an iodine absorption cell for precise
  • h, a recording thermometer, an ultra-violet spectrograph, and an air sampler.
  • gh Accuracy Radial Velocity Planet Searcher spectrograph apparatus (HARPS) at the La Silla Observato
  • acy Radial Velocity Planet Searcher (HARPS) spectrograph at the Chile-based La Silla Observatory.
  • of California, Berkeley using the Hamilton Spectrograph at the Lick Observatory near San Jose in Ca
  • These observations were made with a spectrograph attached to the 13-inch Fitz-Clark refracti
  • He invented the feathering spectrograph by using the commonly occurring chromatic a
  • (GUVI): A spatial-scanning, far-ultraviolet spectrograph designed to globally measure the compositio
  • The spectrograph, developed by UCLA and Montreal, images and
  • g 1 square degree on the sky, while the B&C Spectrograph does spectroscopy.
  • A high resolution Coude spectrograph exists but is currently not operational.
  • s gamma-ray bursts; and the high-resolution spectrograph, FEROS, used to make detailed studies of st
  • imaging and a fiber-fed visible wavelength spectrograph, FOBOS, for general spectroscopy and precis
  • Low-resolution spectrograph for 10-100 μm
  • ned and oversaw construction of a Newtonian spectrograph for the 74-inch (1.9 m) Radcliffe Telescope
  • Meudon, France, which has in its interior a spectrograph for examination of the sun.
  • - such as the recent addition of the Beeman spectrograph for metallurgists - necessitating the Outwo
  • ing instruments, including an early speckle spectrograph for obtaining spatially resolved spectra at
  • lities Council to work on a high-resolution spectrograph for the Gemini telescope in Chile, which pr
  • covered by measurements taken by the ELODIE spectrograph from 2005 and 2006, and later confirmed by
  • ctric photometer and the Boller and Chivens spectrograph have not been in use for more than a decade
  • On January 7, 2007, Bonfils used the HARPS spectrograph in ESO and found an intermediate mass plane
  • ELODIE was an echelle type spectrograph installed at the Observatoire de Haute-Prov
  • Spectrograph is a closely related term.
  • The CORALIE spectrograph is an echelle type spectrograph used for as
  • The low-resolution spectrograph is housed at the prime focus, while the med
  • the tower by hiding it behind crates in the spectrograph lab.
  • ed this planet in early 2007 by using HARPS spectrograph located in Chile.
  • ed this planet in March 2007 by using HARPS spectrograph located in Chile.
  • ed this planet in early 2007 by using HARPS spectrograph located in Chile.
  • ted the construction of an infrared imaging spectrograph, Mimir, in collaboration with Dan Clemens o
  • unced on January 7, 2007 by using the HARPS spectrograph mounted on the ESO's 3.6 meter telescope at
  • ian astronomical institutes using the VIMOS spectrograph, mounted on the telescope Melipal (UT3) of
  • l velocity method using the CORALIE Echelle spectrograph mounted on the 1.2 meter Euler Swiss Telesc
  • SUPOS, Sunrise Polarimetric Spectrograph observes the Zeeman splitting of the calciu
  • lanet Search Program using the MIKE echelle spectrograph on the 6.5-m Magellan II (Clay) telescope.
  • Observations carried out with the UVES spectrograph on COROT-7b in and out of transit, searchin
  • r 26, 2008 by Moutou et al. using the HARPS spectrograph on ESO's 3.6 meter telescope installed at L
  • oject and investigated further by the HARPS spectrograph on ESO's 3.6-metre telescope at La Silla, G
  • e Monitoring Sets) and the SRS (Solar Radio Spectrograph Radiometer).
  • focused on the design of the very sensitive spectrograph required to detect extrasolar planets by de
  • The light is guided to a spectrograph room under the main telescope where a CCD c
  • rror used to focus ultraviolet light onto a spectrograph situated at the prime focus.
  • overed by using radial velocity method from spectrograph taken at Keck Observatory on November 13, 2
  • et Hitchhiker (IEH-02), and the Ultraviolet Spectrograph Telescope for Astronomical Research (UVSTAR
  • The Crossley telescope utilized a slitless spectrograph that was originally employed by Nicholas Ma
  • metry, the Compton edge is a feature of the spectrograph that results from the Compton scattering in
  • Using the low-resolution spectrograph, the telescope has been used to identify Ty
  • for astronomy, and runs the CORALIE echelle spectrograph to search for planets.
  • as-discharge and scintillation counters), a spectrograph to study ozone absorption bands, and a micr
  • f 0.01 per cent; a high spectral resolution spectrograph to obtain spectra in 5 widely separated abs
  • An echelle spectrograph uses two diffraction gratings, rotated 90 d
  • HYDRA: HYDRA is a multiobject spectrograph using fiber optics positioned in the focal
  • Spectrograph: Wadsworth
  • The Faint Object Spectrograph was one of the 4 original axial instruments
  • tly to form a 16-m equivalent telescope the spectrograph will reach extremely faint objects.