We used early data from the Herschel Astrophysical Terahertz Large Area Survey to demonstrate that wide -
area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100 % efficiency.
Not exact matches
Another plan Rubio is working on is developing the Atacama Astronomical Park, a 36,347 - hectare protected
area around the Atacama Large Millimeter /
submillimeter Array, which CONICYT plans to use to attract future telescopes from Brazil and the United States, and maybe also from China, South Korea and Thailand.
Using data from the Herschel Space Telescope, Negrello et al. (p. 800) showed that by searching for the brightest sources in a wide enough
area in the sky it was possible to detect gravitationally lensed
submillimeter galaxies with nearly full efficiency.
The Atacama Large Millimeter /
Submillimeter Array (ALMA) has been conceived as a radio telescope comprised of sixty - four transportable 12 - meter diameter antennas distributed over an
area 14 km in extent.
The combined
area of all antennas used to collect signals from celestial objects is more than 40 times larger than that available to astronomers using existing
submillimeter telescopes.
Abstract: We use new large
area far infrared maps ranging from 65 - 500 microns obtained with the AKARI and the Balloon - borne Large Aperture
Submillimeter Telescope (BLAST) missions to characterize the dust emission toward the Cassiopeia A supernova remnant (SNR).
Using the AKARI high resolution data we find a new «tepid» dust grain population at a temperature of ~ 35K and with an estimated mass of 0.06 sola... ▽ More We use new large
area far infrared maps ranging from 65 - 500 microns obtained with the AKARI and the Balloon - borne Large Aperture
Submillimeter Telescope (BLAST) missions to characterize the dust emission toward the Cassiopeia A supernova remnant (SNR).