The K-band multi-object spectrograph, or KMOS for short, is an instrument mounted on ESO’s Very Large Telescope Antu (UT1) at the Paranal Observatory in...

including the KMOS (K-band multi-object spectrograph) and the VIMOS (Visible Multi Object Spectrograph) instruments, have multi-object spectroscopic capabilities...

or KMOS. KMOS KMOS (K-band Multi Object Spectrograph) is a cryogenic near-infrared multi-object spectrometer, observing 24 objects simultaneously, intended...

An optical spectrometer (spectrophotometer, spectrograph or spectroscope) is an instrument used to measure properties of light over a specific portion...

(2014-07-08). "Performance of the K-band multi-object spectrograph (KMOS) on the ESO VLT". In Ramsay, Suzanne K.; McLean, Ian S.; Takami, Hideki (eds...

instrument is a multi-object spectrograph and is capable of simultaneously measuring the near-infrared spectrum of up to 100 objects like stars or galaxies...

The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a scientific instrument for infrared astronomy, installed on the Hubble Space Telescope...

Infrared Camera and Multi-Object Spectrometer (NICMOS; 1997–present, hibernating since 2008) Space Telescope Imaging Spectrograph (STIS; 1997–present...

corrective-optics module in the Hubble Space Telescope in 1993, the Hubble Faint Object Spectrograph (FOS) was used to measure the rotation velocity of the ionized gas...

spectra, or other observations of objects that share a common type or feature. Surveys are often restricted to one band of the electromagnetic spectrum...

light was obtained on the Kecks I telescope on April 4, 2012. A multi-object spectrograph wide-field camera for the near-infrared (0.97 to 2.41 μm), its...

PDS 70 c, was discovered in 2019 using the VLT's MUSE integral field spectrograph. The planet orbits its host star at a distance of 34.3 AU (5.13 billion...

An object with the spectral type L (also called L-dwarf) can be either a low-mass star, a brown dwarf or a young free-floating planetary-mass object. If...

of celestial objects in deep space. GMT-Consortium Large Earth Finder (G-CLEF) – an optical-band echelle spectrograph GMT Multi-object Astronomical and...

scheduled for launch in 2025 WFMOS – (instrumentation) Wide-Field Multi-Object Spectrograph, proposed instrument for the Gemini telescopes WFPC – (instrumentation)...

from one optical table to another. One mode is a spectrograph mode, using the TRIPPEL spectrograph. The other mode is an imaging mode, where the beam...

each band of the spectrum that is captured. If the scanner detects a large number of fairly narrow frequency bands, it is possible to identify objects even...

Observatory. The multi-object mode relies on a complex micro-shutter mechanism to allow for simultaneous observations of hundreds of individual objects anywhere...

astronomy is the observation of the instant one celestial object occults or eclipses another. Multi-chord asteroid occultation observations measure the profile...

32 K (−241.2 °C; −402.1 °F) and 37 K (−236.2 °C; −393.1 °F). The Focal Plane Electronics operate at 290 K. NIRCam should be able to observe objects as...

60-inch telescope currently[when?] hosts the SED Machine integral field spectrograph instrument used as part of ZTF transient followup and classification...

Walker at the Lick Observatory, using the 120-inch telescope, coudé Spectrograph, and Lallemand electronographic camera. They estimated the mass of the...

slit and multi-object slit-masks. Mounted at Cassegrain focus. WEAVE WHT Enhanced Area Velocity Explorer - a multi-object optical spectrograph, which uses...

self-luminous objects by spectral type, a distinction intimately tied to the surface temperature, and brown dwarfs occupy types M (2100–3500 K), L (1300–2100 K),...

Survey in 2000. These objects show weaker CH4 absorption than previously discovered T-dwarfs. CH4 appears first in the K-band in L8 dwarfs and L- and...

equinoxes primary The main physical body of a gravitationally bound, multi-object system. The primary constitutes most of the system's mass and is generally...

Its discovery image in the i-band was taken on the night of 23 February 2013 with the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope...

time; from the 1990s, the development of fibre-optic spectrographs and multi-slit spectrographs enabled spectra for several hundred galaxies to be observed...

simultaneously imaged by the Space Telescope Imaging Spectrograph (STIS) and the Near Infrared Camera and Multi-Object Spectrometer (NICMOS). The rationale behind...

flight hardware was built by NASA Goddard Space Flight Center. Infrared Spectrograph (IRS) An infrared spectrometer with four sub-modules which operate at...