OSIRIS, the OH - Suppressing
Infrared Imaging Spectrograph, is an «integral field spectrograph.»
The first of these was Keck Observatory's instrument OSIRIS (OH - Suppressing
Infrared Imaging Spectrograph) and its advanced adaptive optics (AO) system.
The researchers made their discovery by obtaining spectroscopic measurements of S0 - 2 using W. M. Keck Observatory's OH - Suppressing
Infrared Imaging Spectrograph (OSIRIS) and Laser Guide Star Adaptive Optics.
Not exact matches
Infrared rays collected by the mirror bounce to one of three instruments: an imaging camera, a spectrograph that breaks up infrared light into its constituent wavelengths (creating an infrared rainbow), and a combined camera - spectrograph that studies a somewhat different part of the infrared spectrum than the ot
Infrared rays collected by the mirror bounce to one of three instruments: an
imaging camera, a
spectrograph that breaks up
infrared light into its constituent wavelengths (creating an infrared rainbow), and a combined camera - spectrograph that studies a somewhat different part of the infrared spectrum than the ot
infrared light into its constituent wavelengths (creating an
infrared rainbow), and a combined camera - spectrograph that studies a somewhat different part of the infrared spectrum than the ot
infrared rainbow), and a combined camera -
spectrograph that studies a somewhat different part of the
infrared spectrum than the ot
infrared spectrum than the other two.
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.
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 s
Spectrograph (IRDIS), a multi-purpose camera for
imaging, polarimetry, and long - slit spectroscopy, and the integral field
spectrograph (IFS), an integral field s
spectrograph (IFS), an integral field
spectrographspectrograph.
Our reference differential
imaging (RDI) data anal... ▽ More We present observations of the Herbig Ae star HD169142 with VLT / SPHERE instruments
InfraRed Dual - band Imager and
Spectrograph (IRDIS)($ K1K2 $ and $ H2H3 $ bands) and the Integral Field
Spectrograph (IFS)($ Y$, $ J$ and $ H$ bands).
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.
Abstract: We report on mid - and far - IR Spitzer observations of 7 nearby dusty elliptical galaxies by using the Multiband
Imaging Photometer (MIPS) and
Infrared Spectrograph (IRS).
In order to study the origin and the propertie... ▽ More We report on mid - and far - IR Spitzer observations of 7 nearby dusty elliptical galaxies by using the Multiband
Imaging Photometer (MIPS) and
Infrared Spectrograph (IRS).