Sentences with phrase «near infrared spectrograph»

After finding the candidate, officially named GOODS - N - 774, with an infrared camera on the Hubble Space Telescope, team members flew to Hawaii on the night of January 11, 2014 and actually saw the formation process underway with the Near Infrared Spectrograph (NIRSPEC) instrument installed on Keck Observatory's 10 - meter Keck II telescope.

ESA's contributions to JWST include the Near Infrared Spectrograph (NIRSpec), the Mid-Infrared Instrument (MIRI) Optics Assembly, and the Ariane 5 Launch Vehicle.

The team used the Gemini - North telescope in Hawaii and the Gemini Near Infrared Spectrograph to observe WISE 0855 over 13 nights for a total of about 14 hours.

The microshutters were moved into a NASA Goddard cleanroom for testing to verify they work correctly before being installed in the Webb's Near Infrared Spectrograph (NIRSpec) instrument.

Not exact matches

The MOIRCS near - infrared spectrograph is very effective for studies focused on the distant, early universe because strong emission lines from star - forming galaxies are redshifted from the optical to the near - infrared regime.

At the American Astronomical Society meeting here, excited astronomers presented the first images taken by Hubble's NICMOS (Near - Infrared Camera and Multi-Object Spectrograph) camera after it was outfitted with a new cooling system in March.

Bañados adds that the Gemini Near - Infrared Spectrograph (GNIRS) went beyond what other instruments on other sites can do.

The two, 10 - meter optical / infrared telescopes near the summit of Mauna Kea on the Island of Hawai'i feature a suite of advanced instruments including imagers, multi-object spectrographs, high - resolution spectrographs, integral - field spectrographs and world - leading laser guide star adaptive optics systems.

Those bands were not seen again until 2011 when the the team observed the planet with Keck Observatory's NIRSPEC, a unique, near - infrared spectrograph that combines broad wavelength coverage with high spectral resolution, allowing the observers to clearly see subtle emissions from the bright parts of Saturn.

The two, 10 - meter optical / infrared telescopes near the summit of Mauna Kea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high - resolution spectrographs, integral - field spectographs and world - leading laser guide star adaptive optics systems.

Using data of tau Boo b collected with the Near Infrared Echelle Spectrograph (NIRSPEC) instrument at the W. M. Keck Observatory in Hawai'i, the researchers were able to compare the molecular signature of water to the light spectrum emitted by the planet, confirming that the atmosphere did indeed include water vapor.

Co-author Mike Brown of Caltech in Pasadena, analyzed data collected from the Near - Infrared Echelle Spectrograph (NIRSPEC) and OH Suppressing Infra - Red Imaging Spectrograph (OSIRIS) instruments on the mighty Keck II telescope on Mauna Kea, Hawaii, over four nights in September 2011.

The two, 10 - meter optical / infrared telescopes near the summit of Mauna Kea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high - resolution spectrographs, integral - field spectrographs and world - leading laser guide star adaptive optics systems.

NASA is still awaiting two more contributions: the Near - Infrared Camera (NIRCam) from Lockheed Martin and the University of Arizona, and the Near - Infrared Spectrograph (NIRSpec) from the European Space Agency, which is still in its early testing phases.

A dedicated instrument for the direct detection of planets, SPHERE, is composed of a polametric camera in visible light, the Zurich IMager POLarimeter (ZIMPOL), and two near - infrared sub-systems: the Infra - Red Dual - beam Imager and Spectrograph (IRDIS), a multi-purpose camera for imaging, polarimetry, and long - slit spectroscopy, and the integral field spectrograph (IFS), an integral field sSpectrograph (IRDIS), a multi-purpose camera for imaging, polarimetry, and long - slit spectroscopy, and the integral field spectrograph (IFS), an integral field sspectrograph (IFS), an integral field spectrographspectrograph.

The Canadian Space Agency has also delivered its instrument: the Fine Guidance Sensor / Near InfraRed Imager and Slitless Spectrograph (FGS / NIRISS) that will also take high - quality images of other bodies in space.

IRDIS was operated in parallel with the integral field spectrograph (IFS) of SPHERE to collect low - resolution ($ R \ sim30 $), near - infrared (0.94 - 1.64 $ \ mu $ m) spectra of the two innermost planets HR8799d and e.

«NIRES is expected to be one of the most efficient single - object, near - infrared spectrographs on an eight to ten - meter telescope, designed to study explosive, deep sky phenomena such as supernovae and gamma ray bursts, a capability that is in high demand.»

The two, 10 - meter optical / infrared telescopes near the summit of Mauna Kea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high - resolution spectrographs, integral - field spectroscopy and world - leading laser guide star adaptive optics systems.

Modal noise become significantly more important as the wavelength increases and presents a risk to the new generation of near - infrared precision radial spectrographs under construction or being proposed to search for planets around cool M - dwarf stars, which emit most of their light in the NIR.

To make these fascinating discoveries, the JWST will rely primarily on four scientific instruments: a near - infrared (IR) camera, a near - IR multi-object spectrograph, a mid-IR instrument and a tunable filter imager.

CSA's contributions to JWST include the Fine Guidance Sensor (FGS) and the Near Infrared Imager and Slitless Spectrograph (NIRISS).

This is an increasingly pressing problem for precision radial velocity (RV) spectrographs in the near - infrared (NIR) and optical that require both high stability of the observed line profiles and high signal to noise.

To validate candidate planets identified by K2, the researchers obtained high - resolution images of the planet - hosting stars from Keck Observatory's near infrared camera (NIRC2), the Gemini and Large Binocular Telescope (among others) as well as high - resolution optical spectroscopy using Keck Observatory's high resolution spectrograph (HIRES) instrument and the AUtomated Planet Finder.

We present the design and performance of the Environmental Control System (ECS) for the Habitable - zone Planet Finder (HPF), a high - resolution (R = 50,000) fiber - fed near infrared (NIR) spectrograph for the 10m Hobby Eberly Telescope at McDonald Observatory.

High - resolution observations are presented based on direct imaging, two - dimensional spectropolarimetry with Fabry - Pérot interferometers, and scanning long - slit spectrographs to introduce some of the science cases for high - resolution solar physics: (1) statistical properties of flows in and around pores and sunspots, (2) chromospheric dynamics associated with newly emerging flux, and (3) flare diagnostics from near - infrared spectropolarimetry.

While this fiber system is designed for the Habitable - zone Planet Finder spectrograph, it is more generally applicable to other instruments in the visible and near - infrared.

To accomplish this, the telescope comes equipped with instruments such as the Near - Infrared Camera (NIRCam), the Near - Infrared Spectrograph (NIRSpec), the Mid-Infrared Instrument (MIRI), and the Fine Guidance Sensors / Near - Infrared Imager and Slitless Spectrograph (FGS / NIRISS).

J. C. Wilson, F. Hearty, M. F. Skrutskie et al., The Apache Point Observatory Galactic Evolution Experiment (APOGEE) high - resolution near - infrared multi-object fiber spectrograph, Society of Photo - Optical Instrumentation Engineers (SPIE) Conference Series 7735 (2010) 77351C; adsabs: 2010SPIE.7735 E..46 W; doi: 10.1117 / 12.856708.