Not exact matches
To make the 3 - D map, Milisavljevic and co-author Rob Fesen of Dartmouth College examined Cas A in near -
infrared wavelengths of light using the Mayall 4 - meter
telescope at Kitt Peak National Observatory, southwest of Tucson, AZ..
According to Mather and other leading astronomers now working on a report to be released this summer by the Association of Universities for Research in Astronomy (AURA), that quest and others require an even bigger space
telescope that would observe, as Hubble does,
at optical, ultraviolet and near -
infrared wavelengths.
[1] ESO's VISTA
telescope observed in the near -
infrared wavelength range 0.88 - 2.15 μm while Spitzer performed observations in the mid-
infrared at 3.6 and 4.5 μm.
Early in their lives, the radiation they emitted was largely blocked by the thick veil of their host nebula, visible only to
telescopes at infrared and radio
wavelengths.
The scientists then mapped the quasars with other
telescopes and
at wavelengths ranging from ultraviolet to far
infrared.
Previously, astronomers have used x-ray
telescopes to observe strong winds very near the massive black holes
at galactic centers (artist's concept, inset) and
infrared wavelengths to detect the vast outflows of cool gas (bluish haze in artist's concept, main image) from such galaxies as a whole, but they've never done so in the same galaxy.
The team used the GROND imager
at the 2.2 m ESO / MPG
telescope of the European Southern Observatory in Chile to observe the planet simultaneously
at seven different
wavelength bands spanning the optical and near -
infrared.
The observations have involved dozens of
telescopes around the world and in space and
at wavelengths from visible light through the
infrared to radio.
ALMA will consist of 64 12 - meter - diameter dish antennas comprising a single imaging
telescope to study the universe
at millimeter and submillimeter
wavelengths — the region between radio waves and
infrared waves.
The APEX
telescope in Chile has mapped the full area of the Galactic Plane visible from the southern hemisphere for the first time
at submillimetre
wavelengths — between
infrared light and radio waves — and in finer detail than recent space - based surveys.
Figures 1a and 1b show the G35 protostar
at wavelengths of 31 and 37 microns taken by the FORCAST instrument on the SOFIA observatory's
infrared telescope in 2011.
The
telescope will observe the universe
at millimeter and submillimeter
wavelengths, between
infrared light and radio waves in the electromagnetic spectrum.
ALMA's observations,
at submillimetre
wavelengths, are also impervious to the glare from the star that affects
infrared or visible - light
telescopes.
Both images were taken by Imke de Pater (UC Berkeley), Larry Sromovosky and Pat Fry (U. Wisconsin), and Heidi Hammel (AURA) using the near -
infrared camera NIRC2 with adaptive optics on the 10 - m Keck II
telescope at a
wavelength of 1.6 micron.
The HDST would have comparable clarity
at UV / optical
wavelengths as the giant ground - based
telescopes get in the near
infrared and as ALMA gets
at millimeter
wavelengths.
That altitude is above the primary part of the atmosphere that blocks
infrared light, which means the
telescope can observe
at wavelengths longer than the ones we see in our Disk Detective WISE data, but shorter than the submillimeter
wavelengths we've observed
at with the James Clerk Maxwell
Telescope.
Images of Io obtained
at different
infrared wavelengths (in microns, μm, or millionths of a meter) with the W. M. Keck Observatory's 10 - meter Keck II
telescope on Aug. 15, 2013 (a-c) and the Gemini North
telescope on Aug. 29, 2013 (d).
Telescopes that capture visible and
infrared light typically require mirrors, and developing foldable mirrors for these
wavelengths is complex when it is even possible
at all.
This was necessary because if the
telescope were not cooled down, its own thermal radiation
at infrared wavelengths would swamp the much fainter radiation from astronomical objects.
The third panel shows the same part of sky again
at even shorter
wavelengths, the near -
infrared, as seen by ESO's VISTA
infrared survey
telescope at the Paranal Observatory in Chile.