With sharper tips and improved antenna function, we also hope to
obtain infrared spectra of single proteins in the future.
Now, a team led by astronomers at UC Santa Cruz has succeeded in
obtaining an infrared spectrum of WISE 0855 using the Gemini North telescope in Hawaii, providing the first details of the object's composition and chemistry.
Not exact matches
It involves using a reflectance spectroscopy setup to
obtain optical reflectance
spectra of paper samples in the near -
infrared, visible, and near - ultraviolet wavelength ranges.
Rieke's plans for JWST investigations include imaging nearby debris disks deeply enough to detect young ice giant planets to understand how they sculpt debris disks, and
obtaining multiple epoch
infrared spectra of variable disks.
Fig. 2: Image in the
infrared spectrum near G345.4938 +01.4677
obtained by the VVV project using the VISTA telescope at Cerro Paranal Observatory.
μm)
spectra,
obtained on the 2.7 m Harlan J. Smith Telescope at McDonald Observatory with the Immersion Grating
INfrared Spectrometer (IGRINS)(Park et al. 2014, SPIE, 9147, 1), for a variety of Galactic PDRs including regions of high mass star formation, reflection nebulae, and planetary nebulae.
Our
spectra,
obtained with the
Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope, reveal gas - phase absorption from CO2 (15.0 um), C2H2 (13.7 um) and HCN (14.0 um).
We present and exploit new near -
infrared images and integral - field
spectra of the four gas giants surrounding HR8799
obtained with SPHERE, the new planet finder instrument at the Very Large Telescope, during the commissioning and science verification phase of the instrument (July - December 2014).
We present and exploit new near -
infrared images and integral - field
spectra of the four gas giants surrounding HR8799
obtained with SPHERE, the new planet f... ▽ More The planetary system discovered around the young A-type HR8799 provides a unique laboratory to: a) test planet formation theories, b) probe the diversity of system architectures at these separations, and c) perform comparative (exo) planetology.
The APOGEE survey has
obtained high - resolution
infrared spectra of more than 100,000 stars.
First, PFIR
obtains a fuller
infrared spectrum and a sharper image — 6 - nm spatial resolution — of a wider variety of materials than does SNOM.
With the Fourier Transform Spectrometer of the AKARI / Far -
Infrared Surveyor, we performed the far - infrared (60 - 140 cm ^ -1) spectral mapping of an area of about 10» x 10» which includes the two clusters to obtain a low - resolution (R = 1.2 cm ^ -1) spectrum at every spatial bin of 30» x 30
Infrared Surveyor, we performed the far -
infrared (60 - 140 cm ^ -1) spectral mapping of an area of about 10» x 10» which includes the two clusters to obtain a low - resolution (R = 1.2 cm ^ -1) spectrum at every spatial bin of 30» x 30
infrared (60 - 140 cm ^ -1) spectral mapping of an area of about 10» x 10» which includes the two clusters to
obtain a low - resolution (R = 1.2 cm ^ -1)
spectrum at every spatial bin of 30» x 30».
With the Fourier Transform Spectrometer of the AKARI / Far -
Infrared Surveyor, we performed the far - infrared (60 - 140 cm ^ -1) spectral mapping of an area of about 10» x 10» which includes the two clusters to obtain a low - resolution (R = 1.2 cm ^ -1) spectrum at every spatial bin o... ▽ More We investigate the properties of interstellar dust in the Galactic center region toward the Arches and Quintuplet c
Infrared Surveyor, we performed the far -
infrared (60 - 140 cm ^ -1) spectral mapping of an area of about 10» x 10» which includes the two clusters to obtain a low - resolution (R = 1.2 cm ^ -1) spectrum at every spatial bin o... ▽ More We investigate the properties of interstellar dust in the Galactic center region toward the Arches and Quintuplet c
infrared (60 - 140 cm ^ -1) spectral mapping of an area of about 10» x 10» which includes the two clusters to
obtain a low - resolution (R = 1.2 cm ^ -1)
spectrum at every spatial bin o... ▽ More We investigate the properties of interstellar dust in the Galactic center region toward the Arches and Quintuplet clusters.
This time was different: Cassini's VIMS (Visible and
Infrared Mapping Spectrometer)
obtained spectra of the storm head and its vicinity.