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A Faint Progenitor System for the Faint Supernova 2024vjm
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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
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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
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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.
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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.
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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.
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We wish to give an overview of the background and recent progress on telescoping algorithms developed by Gosper and Zeilberger, et al.
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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
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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
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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
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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.
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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.
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Science, 2001
All astronomy data and literature will soon be online and accessible via the Internet. The community is building the Virtual Observatory, an organization of this worldwide data into a coherent whole that can be accessed by anyone, in any form, from anywhere.
Jim Gray 0001, Alexander S. Szalay
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All astronomy data and literature will soon be online and accessible via the Internet. The community is building the Virtual Observatory, an organization of this worldwide data into a coherent whole that can be accessed by anyone, in any form, from anywhere.
Jim Gray 0001, Alexander S. Szalay
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Medium-sized telescopes for the Cherenkov Telescope Array
SPIE Proceedings, 2014CTA, the Cherenkov Telescope Array, is the next generation ground-based observatory for gamma-ray astronomy in the energy range from 20 GeV to 300 TeV. The sensitivity in the core energy range will be dominated by up to 40 Medium- Sized Telescopes. These telescopes, of Davies-Cotton type with a reflector with a diameter of 12 m, are currently in the ...
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