Results 261 to 270 of about 128,513 (313)
Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab
Santos Ld +13 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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 +1 more source
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 +1 more source
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 +1 more source
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 +1 more source
Proceedings of the 2019 International Symposium on Symbolic and Algebraic Computation, 2019
We wish to give an overview of the background and recent progress on telescoping algorithms developed by Gosper and Zeilberger, et al.
openaire +1 more source
We wish to give an overview of the background and recent progress on telescoping algorithms developed by Gosper and Zeilberger, et al.
openaire +1 more source
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.
V, Greco, G, Molesini, F, Quercioli
openaire +2 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.
V, Greco, G, Molesini, F, Quercioli
openaire +2 more sources
Multiple mirror telescope as a phased array telescope
Applied Optics, 1985By adjusting the optical path lengths of its individual beams, it is possible to make the multiple mirror telescope (MMT) into a phased array with a 6.86-m base line. A coherent phased focus can be achieved with tilted focal planes if the tilt angle is chosen so that the internal phase differences exactly compensate the external phase differences. This
E K, Hege +3 more
openaire +2 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 +2 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 +2 more sources