Sentences with phrase «observations at infrared wavelengths»
However, ground - based telescopic observations at infrared wavelengths have not yet detected the planet.
http://solarviews.com/ Not exact matches
Because these extremely faint stars are brightest at near - infrared wavelengths of light, the team emphasized that this type of observation could only be accomplished with Hubble's infrared sensitivity to extraordinarily dim light.
[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.
Between January 2003 and November 2011, researchers made more than 40 observations of Jupiter's moon Io at near - infrared wavelengths, shown above at right and the region of Io where they took place, outlined in white at left.
Observations at x-ray and infrared wavelengths didn't reveal any big objects in the cloud.
Observations of a nearby star at infrared wavelengths may capture the ongoing birth of a planet.
«Observations at different wavelengths across the infrared spectrum allow us to piece together a three dimensional picture of how energy and material are transported upwards through the atmosphere.»
More observations are needed, especially at shorter infrared wavelengths than IRAS, says Assendorp.
The observations have involved dozens of telescopes around the world and in space and at wavelengths from visible light through the infrared to radio.
This site provides the exceptionally dry atmospheric conditions necessary for astronomical observations at millimeter and submillimeter wavelengths (wavelengths between the radio and far - infrared spectral regions).
ALMA's observations, at submillimetre wavelengths, are also impervious to the glare from the star that affects infrared or visible - light telescopes.
The photodetector array camera and spectrometer (PACS) aboard the Herschel Space Observatory allows imaging observations in the far infrared at unprecedented resolution, i.e. at better than 6» to 12» over the wavelength range of 60 -LCB- \ mu -RCB- m to 210 -LCB- \ mu -RCB- m. Together with the results from ground - based observations, these spatially resolved data can be modelled to determine the nature of the debris and its evolution more reliably than would be possible from unresolved data alone.
As part of the DUNES and DEBRIS surveys, we obtained observations of three debris disc stars, HIP 22263 (HD 30495), HIP 62207 (HD 110897), and HIP 72848 (HD 131511), at far - infrared wavelengths with the Herschel PACS instrument.
In this NASA & ESA Hubble Space Telescope image of NGC 7479 — created from observations at visible and near - infrared wavelengths — the tightly wound arms of the spiral galaxy create an inverted «S», as they spin in an anticlockwise direction.