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Gotowe bibliografie tematyczne / Automated patrol telescope

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Gotowa bibliografia na temat „Automated patrol telescope”

Autor: Grafiati

Data publikacji: 4 czerwca 2021

Data aktualizacji: 13 lutego 2022

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Artykuły w czasopismach na temat "Automated patrol telescope"

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Cochrane, J. W., P. Mitchell, P. W. Payne, J. W. V. Storey, and B. L. Webster. "The automated patrol telescope." Symposium - International Astronomical Union 118 (1986): 85–86. http://dx.doi.org/10.1017/s0074180900151101.

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A new astronomical system is nearing completion at U.N.S.W. in which a charge coupled device (CCD) array detector is matched to a Schmidt telescope, with the observations completely analyzed on-line. We have modified a Baker-Nunn satellite tracking camera, with its excellent 0.5m, f/1 super-Schmidt optics, converting it into a computer-controlled equatorially-mounted astronomical telescope. The telescope is expected to be located at Siding Spring Observatory in north-western New South Wales.

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Carter, B. D., M. C. B. Ashley, C. S. Bembrick, P. W. Brooks, P. Mitchell, and J. W. V. Storey. "Astronomy with the Automated Patrol Telescope." International Astronomical Union Colloquium 148 (1995): 44–47. http://dx.doi.org/10.1017/s0252921100021667.

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AbstractThe Automated Patrol Telescope (APT) is a wide-field CCD imaging telescope operated by the University of New South Wales at Siding Spring Observatory in Australia. The optical design employed resembles that of a Schmidt, but uses a 3-element lens to achieve a wide, corrected field of view. The APT was developed by extensively modifying the optical, mechanical and electronic systems of a Baker-Nunn satellite tracking camera. Telescope motion and operation of the CCD have been placed under computer control, allowing automated observations for longterm survey and monitoring projects. The

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Brooks, P. W. "Preliminary Results from the Automated Patrol Telescope CCD Camera." Publications of the Astronomical Society of Australia 8, no. 04 (1990): 377–80. http://dx.doi.org/10.1017/s132335800002378x.

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Abstract The University of NSW Automated Patrol Telescope (APT), a modified 0.5 m Baker-Nunn Schmidt telescope situated at Siding Spring Observatory, Coonabarabran, Australia, was opened in June 1989. It features the unique combination of an extremely fast (f/1) optical system with a CCD (Charge-Coupled Device) camera at the prime focus, capable of both fast (50 Hz TV-rate) imaging and slow-scan integrated readout via a low noise Correlated Double Sampling amplifier. This combination of optics and detector gives a wide field (0.9° × 1.4°) suited to observing extended objects including the LMC,

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Carter, B. D., C. S. Bembrick, M. C. B. Ashley, and P. Mitchell. "The university of New South Wales automated patrol telescope." Experimental Astronomy 5, no. 1-2 (March 1994): 81–85. http://dx.doi.org/10.1007/bf01583814.

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Mitchell, P., and E. Ollier. "TV Rate Readout Unit for Two-dimensional CCDs." Publications of the Astronomical Society of Australia 7, no. 1 (1987): 36–37. http://dx.doi.org/10.1017/s1323358000021792.

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AbstractA simple circuit has been designed for reading out at TV rate the two-dimensional CCD on the Automated Patrol Telescope. Because it is controlled by a programmable Cathode Ray Tube Controller integrated circuit it is very flexible and applicable to frame transfer CCDs having a wide range of formats.

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Yim, Hong-Suh, Myung-Jin Kim, Young-Ho Bae, Hong-Kyu Moon, Young-Jun Choi, Dong-Goo Roh, Jintae Park, and Bora Moon. "DEEP-South: Automated Observation Scheduling, Data Reduction and Analysis Software Subsystem." Proceedings of the International Astronomical Union 10, S318 (August 2015): 311–12. http://dx.doi.org/10.1017/s1743921315007243.

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AbstractWe started ‘DEep Ecliptic Patrol of the Southern sky’ (DEEP-South, DS) (Moon et al. 2015) in late 2012, and conducted test runs with the first Korea Microlensing Telescope Network (KMTNet) (Park et al. 2012), a 1.6 m telescope with 18k x 18k CCD stationed at CTIO in early 2015. While the primary objective of DEEP-South is the physical characterization of small Solar System bodies, it is also expected to discover a large number of such bodies, many of them previously unknown. An automated observation scheduling, data reduction and analysis software subsystem called ‘DEEP-South Schedulin

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Payne, Paul. "Sky Brightness and Atmospheric Extinction at A.N.R.A.O., Parkes and Siding Spring Observatory." Publications of the Astronomical Society of Australia 6, no. 2 (1985): 182–86. http://dx.doi.org/10.1017/s1323358000018051.

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AbstractIn May 1984 site testing began for the Automated Patrol Telescope. A series of atmospheric extinction and night sky brightness measurements were made over the following year at Parkes and Siding Spring Mountain using B and V filters. Parkes revealed an extinction greater than that of Siding Spring and more prone to variation. Results for the night sky brightness indicated Parkes has a sky slightly brighter than that at Siding Spring. The paper discusses the procedures used for obtaining the results and their limitations.

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Steel, Duncan. "Asteroid Discovery Efficiencies for Telescope Systems at Siding Spring." Publications of the Astronomical Society of Australia 12, no. 2 (August 1995): 202–14. http://dx.doi.org/10.1017/s1323358000020282.

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AbstractRelative efficiencies for the discovery of Earth-crossing asteroids (ECAs) are modelled for various telescopes at Siding Spring. It is found that the narrow-field instruments—the Anglo-Australian Telescope and the 40 in and 2·3m reflectors—are not competitive in this regard for present CCD imaging systems. The UK Schmidt Telescope (UKST), if used to take short-exposure stereo pairs of photographs, would be an effective search tool, outperforming all current systems apart from the Ground-based Electro-Optical Deep Space Surveillance (GEODSS) systems now being implemented by the US Air F

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Carter, B. D., M. C. B. Ashley, Y.-S. Sun, and J. W. V. Storey. "Redesigning a Baker-Nunn Camera for CCD Imaging." Publications of the Astronomical Society of Australia 10, no. 1 (1992): 74–76. http://dx.doi.org/10.1017/s1323358000019305.

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AbstractThe University of NSW’s Automated Patrol Telescope is a modified Baker-Nunn satellite tracking camera, now used for CCD imaging of astronomical objects. The f/1 Baker-Nunn optical design gives a 30° field of view with an approximately spherical focal surface of radius ≈500 mm. While the focal plane curvature is tolerable across the 1.4° × 1.0° field of the present CCD, it becomes unacceptable when a larger CCD is used. In addition, the use of glass filters in the highly convergent beam produces intolerable spherical aberration. We present a design modification to the original Baker-Nun

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Wada, Takehiko, Munetaka Ueno, Toshikazu Ebisuzaki, and Yosuke Ohno. "A Near Infrared Survey of the LMC." Symposium - International Astronomical Union 186 (1999): 59. http://dx.doi.org/10.1017/s0074180900112264.

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We surveyed the central 3° × 6° region of the Large Magellanic Cloud (LMC) with angular resolution of 10″.0 at the J(1.25μm), H(1.65μm) and K′(2.15μm) bands. The observations were performed from Oct to Nov, 1994 at the Siding Spring Observatory. We used a 25 cm/F3.5 Newtonian telescope equipped with a 512×512 PtSi-Camera (Ueno et al. 1992). The plate scale was 4.″6 × 6.″0/pixel and the total field of view was 40.′2 × 52.′3. The system was attached onto the Automated Patrol Telescope of the University of New South Wales. The limiting magnitudes of the survey were 13.6, 11.9, and 10.0 magnitude

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Rozprawy doktorskie na temat "Automated patrol telescope"

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Hidas, M??rton Gergely Physics Faculty of Science UNSW. "A search for transiting extrasolar planets with the automated patrol telescope." Awarded by:University of New South Wales. School of Physics, 2005. http://handle.unsw.edu.au/1959.4/22803.

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In the past decade some 150 planets have been detected outside our Solar System, mostly via precise radial-velocity measurements of their host stars. Using an alternative method, transit searches have recently added 6 planets to the tally, and are expected to make more significant contributions in the future. The transit method is based on the detection of the tiny, periodic dip in the apparent brightness of a star when an orbiting planet passes in front of it. It requires intensive photometric monitoring of ??? 104 stars, with a precision better than ??? 1%. The 0.5 m Automated Patrol Telesco

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Hamacher, Duane Willis Physics Faculty of Science UNSW. "A search for transiting extrasolar planets from the southern hemisphere." Publisher:University of New South Wales. Physics, 2008. http://handle.unsw.edu.au/1959.4/40943.

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To date, more than 300 planets orbiting stars other than our sun have been discovered using a range of observing techniques, with new discoveries occuring monthly. The work in this thesis focused on the detection of exoplanets using the transit method. Planets orbiting close to their host stars have a roughly 10 per cent chance of eclipsing (transiting) the star, with Jupiter?sized planets causing a one per cent dip in the flux of the star over a few hours. A wealth of orbital and physical information on the system can be extracted from these systems, including the planet density which is esse

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Części książek na temat "Automated patrol telescope"

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Cochrane, J. W., P. Mitchell, P. W. Payne, J. W. V. Storey, and B. L. Webster. "The Automated Patrol Telescope." In Instrumentation and Research Programmes for Small Telescopes, 85–86. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-010-9433-7_14.

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Streszczenia konferencji na temat "Automated patrol telescope"

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Grossan, Bruce, Saul Perlmutter, and Michael Ashley. "A search for gamma-ray burst optical emission with the automated patrol telescope." In GAMMA-RAY BURSTS. ASCE, 1998. http://dx.doi.org/10.1063/1.55461.

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Miziarski, Stan, Michael C. B. Ashley, Greg Smith, Sam Barden, John Dawson, Anthony Horton, Will Saunders, et al. "Big innovations in a small instrument: technical challenges in a new CCD system design for the Automated Patrol Telescope." In SPIE Astronomical Telescopes + Instrumentation, edited by Eli Atad-Ettedgui and Dietrich Lemke. SPIE, 2008. http://dx.doi.org/10.1117/12.788624.

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Bettonvil, Felix C. M. "Remote and automatic small-scale observatories: experience with an all-sky fireball patrol camera." In SPIE Astronomical Telescopes + Instrumentation, edited by Suzanne K. Ramsay, Ian S. McLean, and Hideki Takami. SPIE, 2014. http://dx.doi.org/10.1117/12.2057100.

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