Results 321 to 330 of about 501,201 (339)
Some of the next articles are maybe not open access.
Astronomische Nachrichten, 2001
AbstractThe Liverpool Telescope is a 2.0 metre robotic telescope on La Palma. It achieved first light in July 2003, and began science operations in January 2004, with (supervised) robotic operation from April 2004. Unmanned operation is planned for October 2004.
openaire +2 more sources
AbstractThe Liverpool Telescope is a 2.0 metre robotic telescope on La Palma. It achieved first light in July 2003, and began science operations in January 2004, with (supervised) robotic operation from April 2004. Unmanned operation is planned for October 2004.
openaire +2 more sources
IEEE Instrumentation & Measurement Magazine, 2014
Interferometric gravitational wave detectors are amongst the most sensitive instruments ever built. They are hunting for tiny oscillations in space-time originating from cosmic events such as inspiraling objects or supernova explosions. These detectors are based on Michelson-like interferometers reaching sensitivities for lengths changes of better than
Stefanie Kroker, Ronny Nawrodt
openaire +3 more sources
Interferometric gravitational wave detectors are amongst the most sensitive instruments ever built. They are hunting for tiny oscillations in space-time originating from cosmic events such as inspiraling objects or supernova explosions. These detectors are based on Michelson-like interferometers reaching sensitivities for lengths changes of better than
Stefanie Kroker, Ronny Nawrodt
openaire +3 more sources
2012
Before any imaging can be undertaken the mount must be placed on a solid footing. The strongest, most accurate mount in the world will be no good for astroimaging if it wobbles because it is not securely in contact with the ground. If the mount is supported by a tripod then placing it on something solid is preferable to placing it directly onto grass ...
Stephen Chadwick, Ian Cooper
openaire +2 more sources
Before any imaging can be undertaken the mount must be placed on a solid footing. The strongest, most accurate mount in the world will be no good for astroimaging if it wobbles because it is not securely in contact with the ground. If the mount is supported by a tripod then placing it on something solid is preferable to placing it directly onto grass ...
Stephen Chadwick, Ian Cooper
openaire +2 more sources
Applied Optics, 1993
The Florentine Istituto e Museo di Storia delta Scienza houses two complete telescopes and a single objective lens (reconstructed from several fragments) that can be attributed to Galileo. These optics have been partially dismantled and made available for optical testing with state-of-the-art equipment.
Franco Quercioli +2 more
openaire +3 more sources
The Florentine Istituto e Museo di Storia delta Scienza houses two complete telescopes and a single objective lens (reconstructed from several fragments) that can be attributed to Galileo. These optics have been partially dismantled and made available for optical testing with state-of-the-art equipment.
Franco Quercioli +2 more
openaire +3 more sources
AIP Conference Proceedings, 2002
Neutrino telescopes complement gamma ray telescopes in the observations of energetic astronomical sources as well as in searching for the dark matter. This paper gives the status of the current generation neutrino telescopes projects: Baikal, AMANDA, NESTOR, NEMO and ANTARES with particular emphasis on the ANTARES telescope in the Mediterranean Sea.
openaire +1 more source
Neutrino telescopes complement gamma ray telescopes in the observations of energetic astronomical sources as well as in searching for the dark matter. This paper gives the status of the current generation neutrino telescopes projects: Baikal, AMANDA, NESTOR, NEMO and ANTARES with particular emphasis on the ANTARES telescope in the Mediterranean Sea.
openaire +1 more source
Science, 1967
In stellar astronomy, the future of automation techniques lies in their application to the largest telescopes. In such a case, the cost of automation is small compared to that of the telescope project as a whole, and is well repaid in the savings in observing time.
openaire +3 more sources
In stellar astronomy, the future of automation techniques lies in their application to the largest telescopes. In such a case, the cost of automation is small compared to that of the telescope project as a whole, and is well repaid in the savings in observing time.
openaire +3 more sources
The Microscope and the Telescope [PDF]
Journal of Public Health Dentistry, 1983 openaire +2 more sources