Relevant bibliographies by topics / Instrumentation for Astronomy

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Instrumentation for Astronomy'

Author: Grafiati
Published: 9 March 2023
Last updated: 10 March 2023

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Journal articles on the topic "Instrumentation for Astronomy"

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McLean, Ian S., Ding-Qiang Su, Thomas Armstrong, Noah Brosch, Martin Cullum, Michel Dennefeld, George Jacoby, et al. "Commission 9: Instrumentation and Techniques: (Instrumentation et Techniques)." Transactions of the International Astronomical Union 24, no. 1 (2000): 316–27. http://dx.doi.org/10.1017/s0251107x00003266.

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The last triennium, and coincidentally the last few years of the 20th century, has been a most remarkable time for Commission 9, and for astronomy in general. Ground-based astronomy in particular has received an enormous boost due to the arrival of an astonishing array of new telescopes, novel instruments and innovative techniques. For those of us closely involved in developing new observatories, instrumentation or detectors, the last few years have been rather hectic! As an astronomer with a long-time interest in the development of new instruments, what amazes me is the breadth of technology and the visionary scope of all these incredible new achievements. Many of the very large 8-10 meter class telescopes are now coming into full operation – yet, just as this is happening, numerous smaller “survey” telescopes are providing a wealth of new sources. Adaptive optics is being practiced at many sites and diffraction-limited imaging from the ground is now a reality. Several optical-IR interferometers are now working and more are coming along very soon. Detectors continue to get bigger and better, especially for the infrared, and instrumentation is increasingly more sophisticated, complex and efficient. Remote observing, robotic telescopes and global networks of telescopes are common, and international collaborations are larger and stronger than ever before.
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Knödlseder, J. "Instrumentation for gamma-ray astronomy." EAS Publications Series 7 (2003): 1. http://dx.doi.org/10.1051/eas:2003036.

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Webber, J. C., and M. W. Pospieszalski. "Microwave instrumentation for radio astronomy." IEEE Transactions on Microwave Theory and Techniques 50, no. 3 (March 2002): 986–95. http://dx.doi.org/10.1109/22.989982.

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Kurfess, James D. "Perspectives on MeV astronomy instrumentation." New Astronomy Reviews 48, no. 1-4 (February 2004): 177–81. http://dx.doi.org/10.1016/j.newar.2003.11.026.

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Ramsey, Brian D., Robert A. Austin, and Rudolf Decher. "Instrumentation for X-ray astronomy." Space Science Reviews 69, no. 1-2 (July 1994): 139–204. http://dx.doi.org/10.1007/bf00756035.

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Ryan, J. M. "Astrophysics challenges of MeV-astronomy instrumentation." New Astronomy Reviews 48, no. 1-4 (February 2004): 199–204. http://dx.doi.org/10.1016/j.newar.2003.11.052.

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Teegarden, B. J. "Space instrumentation for gamma-ray astronomy." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 422, no. 1-3 (February 1999): 551–61. http://dx.doi.org/10.1016/s0168-9002(98)01268-6.

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Lazareff, B. "Instrumentation for heterodyne mm-wave astronomy." EAS Publications Series 37 (2009): 37–48. http://dx.doi.org/10.1051/eas/0937005.

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Sitarek, Julian. "TeV Instrumentation: Current and Future." Galaxies 10, no. 1 (January 27, 2022): 21. http://dx.doi.org/10.3390/galaxies10010021.

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During the last 20 years, TeV astronomy has turned from a fledgling field, with only a handful of sources, into a fully-developed astronomy discipline, broadening our knowledge on a variety of types of TeV gamma-ray sources. This progress has been mainly achieved due to the currently operating instruments: imaging atmospheric Cherenkov telescopes, surface arrays and water Cherenkov detectors. Moreover, we are at the brink of a next generation of instruments, with a considerable leap in performance parameters. This review summarizes the current status of the TeV astronomy instrumentation, mainly focusing on the comparison of the different types of instruments and analysis challenges, as well as providing an outlook into the future installations. The capabilities and limitations of different techniques of observations of TeV gamma rays are discussed, as well as synergies to other bands and messengers.
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Rosenzweig, Patricia. "Astronomy in Venezuela." Transactions of the International Astronomical Union 24, no. 3 (2001): 205–9. http://dx.doi.org/10.1017/s0251107x00000766.

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AbstractSince the installation of the Observatorio Cagigal in Caracas, astronomy in Venezuela has developed steadily, and, in the last few decades, has been strong. Both theoretical and observational astronomy now flourish in Venezuela. A research group, Grupo de Astrofísica (GA) at the Universidad de Los Andes (ULA) in Mérida, started with few members but now has increased its numbers and undergone many transformations, promoting the creation of the Grupo de Astrofísica Teórica (GAT), the Grupo de Astronomía, the Centro de Astrofísica Teòrica (CAT), and with other collaborators initiated the creation of a graduate study program (that offers master’s and doctor’s degrees) in the Postgrado de Física Fundamental of ULA. With the financial support of domestic Science Foundations such as CONICIT, CDCHT, Fundacite, and individual and collective grants, many research projects have been started and many others are planned. Venezuelan astronomy has benefitted from the interest of researchers in other countries, who have helped to improve our scientific output and instrumentation. With the important collaboration of national and foreign institutions, astronomy is becoming one of the strongest disciplines of the next decade in Venezuela.
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Dissertations / Theses on the topic "Instrumentation for Astronomy"

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Martindale, Adrian. "Novel X-ray instrumentation for astronomy." Thesis, University of Leicester, 2008. http://hdl.handle.net/2381/3964.

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This thesis describes experimental and theoretical work and technology development directed towards the next generation of X-ray astronomical instrumentation. A great heritage exists of instruments which are sensitive to X-rays which operate on board space based observatories. The next generation of such telescopes will take advantage of the rapid technology advancement of the last four decades of more accurately observe the universe and give greater insight into the objects within it, how they formed and how they will evolve. Chapters 2 and 3 describe the investigation of extremely high speed microchannel plate detectors capable of counting individual photons with a timing accuracy of a few tens of picoseconds (1 ps = 10-12s)at extremely high spatial resolution. Although many early X-ray astronomical instruments were based on MCP detectors, it is only recent manufacturing improvements which have enabled the production of such small pore diameters, enabling the unparalleled temporal and spatial resolution. Prospects for future application exist in fields as diverse as X-ray and ultraviolet astronomy and the life sciences. Chapters 4 and 5 report the testing of Microchannel plates as low mass X-ray optics where the development of square pore geometrics has made true imaging MCP telescopes possible. Two flight programs are identified as areas where such optics will provide tangible benefits: These are BepiColombo, a European mission to the planet Mercury which will contain the first ever imaging X-raytelescope on a planetary science mission and Lobster-ISS, a wide field of view telescope for X-ray astronomy which will provide coverage of, almost, the whole sky every 90 minute orbit. Testing reported herein finds that the manufacturing techniques are maturing to a point where they can exceed the <5 arcmin resolution required for these missions. Chapters 6 and 7 comprise a description of a completely novel X-ray polarimeter. For the past three decades, little or now progress has been made in the field of X-ray astrophysical polarimetry owing to the lack of suitable instrumentation, this is despite intense scientific interest in such measurements. A simple optical design for a polarimeter is made possible using highly ordered materials which exhibit dichroism at fixed, narrow energy bands, for the first time allowing simultaneous measurement of ALL astronomically pertinent observables. The areas of science influenced by these three areas of instrument development are shown to be very broad, including; astrophysics and cosmology, planetary science, life sciences, nano-science and even fundamental chemistry.
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Lee, Aizeret, University of Western Sydney, of Science Technology and Environment College, and School of Engineering and Industrial Design. "Radioastronomical instrumentation : the diagonal horn." THESIS_CSTE_EID_Lee_A.xml, 2002. http://handle.uws.edu.au:8081/1959.7/699.

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The horn plays an elemental role in the make up of a radio-telescope. The focus of this research is on one particular type of horn – the diagonal horn. An analysis of the diagonal horn is made using the Fourier method. The analysis begins from Maxwell’s equations, as the basic building block, and describes the steps involved in developing the radiation pattern. Based on the theory, a program was written that produces the theoretical graphs referred to throughout the thesis. A diagonal horn was manufactured and the radiation patterns were measured. A comparison of these measured patterns is made against the theoretically generated patterns. Further research was carried out to demonstrate the effects on the radiation patterns when the horn is fitted with a dielectric plug. This practice may enhance the directivity of the horn at the cost of introducing new losses
Master of Engineering (Hons)
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Price, Daniel Charles. "Radio astronomy instrumentation for redshifted hydrogen line science." Thesis, University of Oxford, 2013. http://ora.ox.ac.uk/objects/uuid:3185b622-9aba-4c0f-995b-eceb50a5a49c.

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This thesis presents instrumentation with which to measure the abundance of neutral hydrogen gas in the Universe. Measuring where the Universe’s hydrogen is, and tracing how its distribution evolves with time, holds the key to understanding how galaxies evolve, the nature of dark energy, and how the first cosmic structures formed. In particular, this thesis looks at instrumentation for 21-cm intensity mapping telescopes. In 21-cm intensity mapping, the collective emission of many galaxies is measured, without individual detections. This technique promises to allow detection of the baryonic acoustic oscillation peaks in the power spectrum of the Universe’s matter distribution. Such a detection would increase constraints on cosmological parameters. There are two main approaches to designing a 21-cm intensity mapping instruments: using a filled aperture instrument such as a single-dish telescope, or using a sparse aperture instrument such as an interferometric array of dipoles. This thesis investigates analogue components for a sparse aperture instrument operating at 1.0-1.5 GHz. As part of this work, a 16-element sparse aperture array was designed and constructed. To test the array’s performance, field testing was conducted; the results of which are presented here. In addition to this, I have designed a new digital spectrometer for redshifted hydrogen line science, named HISPEC. A copy of this spectrometer has been installed on the Parkes 64 m telescope, as a digital signal processor for the 21-cm multibeam receiver. HISPEC has increased instantaneous bandwidth, higher interchannel isolation, and improved quantization efficiency as compared to the existing backend, MBCORR. The HISPEC equipped multibeam receiver is an ideal instrument for 21-cm intensity mapping at redshifts z<0.2.
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McMahon, Peter Leonard. "Adventures in radio astronomy instrumentation and signal processing." Master's thesis, University of Cape Town, 2008. http://hdl.handle.net/11427/5165.

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Includes abstract.
Includes bibliographical references (leaves 117-119).
This thesis describes the design and implementation of several instruments for digitizing and processing analogue astronomical signals collected using radio telescopes. Modern radio telescopes have significant digital signal processing demands that are typically best met using custom processing engines implemented in Field Programmable Gate Arrays. These demands essentially stem from the ever-larger analogue bandwidths that astronomers wish to observe, resulting in large data volumes that need to be processed in real time. We focused on the development of spectrometers for enabling improved pulsar² science on the Allen Telescope Array, the Hartebeesthoek Radio Observatory telescope, the Nançay Radio Telescope, and the Parkes Radio Telescope. We also present work that we conducted on the development of real-time pulsar timing instrumentation.
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Zhang, Shuang Nan. "Instrumentation and data analysis for hard X-ray astronomy." Thesis, University of Southampton, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.252689.

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Baron, Richard Leigh. "Occultation astronomy and instrumentation : studies of the Uranian upper atmosphere." Thesis, Massachusetts Institute of Technology, 1989. http://hdl.handle.net/1721.1/51472.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 1989.
Includes bibliographical references (leaves 207-208).
by Richard Leigh Baron.
Ph.D.
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Charalambous, Andrew. "Opto-mechanical design for large telescope instrumentation." Thesis, University College London (University of London), 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.243313.

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Jovanovic, N., C. Schwab, O. Guyon, J. Lozi, N. Cvetojevic, F. Martinache, S. Leon-Saval, et al. "Efficient injection from large telescopes into single-mode fibres: Enabling the era of ultra-precision astronomy." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/625827.

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Photonic technologies off er numerous advantages for astronomical instruments such as spectrographs and interferometers owing to their small footprints and diverse range of functionalities. Operating at the diffraction-limit, it is notoriously difficult to efficiently couple such devices directly with large telescopes. We demonstrate that with careful control of both the non-ideal pupil geometry of a telescope and residual wavefront errors, efficient coupling with single-mode devices can indeed be realised. A fibre injection was built within the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument. Light was coupled into a single-mode fibre operating in the near-IR (J-H bands) which was downstream of the extreme adaptive optics system and the pupil apodising optics. A coupling efficiency of 86% of the theoretical maximum limit was achieved at 1550 nm for a diffraction-limited beam in the laboratory, and was linearly correlated with Strehl ratio. The coupling efficiency was constant to within <30% in the range 1250-1600 nm. Preliminary on-sky data with a Strehl ratio of 60% in the H-band produced a coupling efficiency into a single-mode fibre of similar to 50%, consistent with expectations. The coupling was >40% for 84% of the time and >50% for 41% of the time. The laboratory results allow us to forecast that extreme adaptive optics levels of correction (Strehl ratio >90% in H-band) would allow coupling of >67% (of the order of coupling to multimode fibres currently) while standard levels of wavefront correction (Strehl ratio >20% in H-band) would allow coupling of >18%. For Strehl ratios <20%, few-port photonic lanterns become a superior choice but the signal-to-noise, and pixel availability must be considered. These results illustrate a clear path to efficient on-sky coupling into a single-mode fibre, which could be used to realise modal-noise-free radial velocity machines, very-long-baseline optical/near-IR interferometers and/or simply exploit photonic technologies in future instrument design.
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Lee, Aizeret. "Radioastronomical instrumentation : the diagonal horn." Thesis, View thesis, 2002. http://handle.uws.edu.au:8081/1959.7/699.

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The horn plays an elemental role in the make up of a radio-telescope. The focus of this research is on one particular type of horn – the diagonal horn. An analysis of the diagonal horn is made using the Fourier method. The analysis begins from Maxwell’s equations, as the basic building block, and describes the steps involved in developing the radiation pattern. Based on the theory, a program was written that produces the theoretical graphs referred to throughout the thesis. A diagonal horn was manufactured and the radiation patterns were measured. A comparison of these measured patterns is made against the theoretically generated patterns. Further research was carried out to demonstrate the effects on the radiation patterns when the horn is fitted with a dielectric plug. This practice may enhance the directivity of the horn at the cost of introducing new losses
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Lee, Hanshin. "Optical Alignment and Novel Instrumentation Techniques for Optical and Near-Infrared Astronomy." Thesis, University of Oxford, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.504421.

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Books on the topic "Instrumentation for Astronomy"

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Leonard, Culhane J., Society of Photo-optical Instrumentation Engineers., Association nationale de la recherche technique., and European Space Agency, eds. X-ray instrumentation in astronomy. Bellingham, Wash., USA: SPIE--the International Society for Optical Engineering, 1986.

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Observational astronomy: Techniques and instrumentation. Cambridge: Cambridge University Press, 2011.

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Robinson, Lloyd B., ed. Instrumentation for Ground-Based Optical Astronomy. New York, NY: Springer New York, 1988. http://dx.doi.org/10.1007/978-1-4612-3880-5.

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1927-, Livingston W. C., ed. Selected papers on instrumentation in astronomy. Bellingham, Wash., USA: SPIE Optical Engineering Press, 1993.

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Electronic imaging in astronomy: Detectors and instrumentation. 2nd ed. Berlin: Springer, 2008.

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Electronic imaging in astronomy: Detectors and instrumentation. Chichester: Wiley, 1997.

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Santa Cruz Summer Workshop in Astronomy and Astrophysics (9th 1987 Lick Observatory). Instrumentation for ground-based optical astronomy: Present and future. Edited by Robinson L. B. New York: Springer-Verlag, 1988.

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1931-, Crawford David Livingstone, Society of Photo-optical Instrumentation Engineers., and American Astronomical Society, eds. Instrumentation in astronomy VIII: 13-14 March 1994, Kona, Hawaii. Bellingham, Wash: SPIE--the International Society for Optical Engineering, 1994.

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C, Mather John, MacEwen Howard A, Graauw, Mattheus W.M. de, American Astronomical Society, and Society of Photo-optical Instrumentation Engineers., eds. Space telescopes and instrumentation I: Optical, infrared, and milllimeter : 24-31 May 2006, Orlando, Florida, USA. Bellingham, Wash: SPIE, 2006.

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Exploration of terrestrial planets from spacecraft: Instrumentation, investigation, interpretation. 2nd ed. Chichester: Wiley, 1997.

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Book chapters on the topic "Instrumentation for Astronomy"

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Auer, Siegfried. "Instrumentation." In Astronomy and Astrophysics Library, 385–444. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56428-4_9.

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Aranda, Ted. "Instrumentation." In Patrick Moore’s Practical Astronomy Series, 13. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-9419-6_4.

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North, Gerald. "Modern Developments in Instrumentation." In Astronomy Explained, 64–76. London: Springer London, 1997. http://dx.doi.org/10.1007/978-1-4471-0901-3_4.

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North, Gerald. "Modern Developments in Instrumentation." In Mastering Astronomy, 66–75. London: Macmillan Education UK, 1988. http://dx.doi.org/10.1007/978-1-349-19604-3_4.

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Dicati, Renato. "The Development of Instrumentation." In Stamping Through Astronomy, 171–202. Milano: Springer Milan, 2013. http://dx.doi.org/10.1007/978-88-470-2829-6_7.

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Wielebinski, Richard, and Bernd Klein. "1.2 Radio astronomy and instrumentation." In Landolt-Börnstein - Group VI Astronomy and Astrophysics, 31–67. Berlin, Heidelberg: Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-540-70607-6_2.

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Nicklas, H. "Optical Telescopes and Instrumentation." In Compendium of Practical Astronomy, 59–136. Berlin, Heidelberg: Springer Berlin Heidelberg, 1994. http://dx.doi.org/10.1007/978-3-642-45688-6_4.

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Lemke, Dietrich. "1.3 Infrared instrumentation." In Landolt-Börnstein - Group VI Astronomy and Astrophysics, 68–108. Berlin, Heidelberg: Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-540-70607-6_3.

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Wyatt, William F., and John C. Geary. "UNIXTMand Data Collection in Astronomy." In Instrumentation for Ground-Based Optical Astronomy, 621–27. New York, NY: Springer New York, 1988. http://dx.doi.org/10.1007/978-1-4612-3880-5_62.

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Aspin, Colin. "Future Instrumentation for the Nordic Optical Telescope." In Optical Detectors for Astronomy, 55–56. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5262-4_8.

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Conference papers on the topic "Instrumentation for Astronomy"

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Jones, Barbara, and R. C. Puetter. "Plans For Keck Telescope Instrumentation." In 1986 Astronomy Conferences, edited by David L. Crawford. SPIE, 1986. http://dx.doi.org/10.1117/12.968126.

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Morris, Katherine, Carolyn Atkins, Lucy Reynolds, James Walpole, Bart van de Vorst, Robert M. Snell, Chris Miller, et al. "Additively manufactured flexure for astronomy instrumentation." In Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation V, edited by Roland Geyl and Ramón Navarro. SPIE, 2022. http://dx.doi.org/10.1117/12.2630180.

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Hoffman, Alan W., Elizabeth Corrales, Peter J. Love, Joseph P. Rosbeck, Michael Merrill, Albert Fowler, and Craig McMurtry. "2Kx2K InSb for astronomy." In SPIE Astronomical Telescopes + Instrumentation, edited by James D. Garnett and James W. Beletic. SPIE, 2004. http://dx.doi.org/10.1117/12.555200.

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Moschetti, Manuele, Marco Riva, Matteo Aliverti, Giorgio Pariani, and Giuseppe Sala. "Smart telescope for astronomy." In SPIE Astronomical Telescopes + Instrumentation, edited by Ramón Navarro and James H. Burge. SPIE, 2016. http://dx.doi.org/10.1117/12.2232992.

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Lesser, Michael. "4KX4K detectors for astronomy." In SPIE Astronomical Telescopes + Instrumentation, edited by James D. Garnett and James W. Beletic. SPIE, 2004. http://dx.doi.org/10.1117/12.551437.

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Nelson, Jerry E., and Terry S. Mast. "Optical Design And Instrumentation Of The Keck Observatory." In 1986 Astronomy Conferences, edited by Lawrence D. Barr. SPIE, 1986. http://dx.doi.org/10.1117/12.963531.

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Escoffier, Raymond P., and John C. Webber. "Wideband correlators for radio astronomy." In Astronomical Telescopes & Instrumentation, edited by Thomas G. Phillips. SPIE, 1998. http://dx.doi.org/10.1117/12.317375.

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Sarazin, Marc S. "Eso-Vlt Instrumentation For Site Evluation In Northern Chile." In 1986 Astronomy Conferences, edited by Lawrence D. Barr. SPIE, 1986. http://dx.doi.org/10.1117/12.963520.

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Beaulieu, Mathilde, Sebastien Ottogalli, Olivier Preis, Yves Bresson, Jean-Pierre Rivet, Lyu Abe, and Farrokh Vakili. "Stable Imaging for Astronomy (SIA)." In SPIE Astronomical Telescopes + Instrumentation, edited by Suzanne K. Ramsay, Ian S. McLean, and Hideki Takami. SPIE, 2014. http://dx.doi.org/10.1117/12.2057529.

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Biondi, Federico, Demetrio Magrin, Roberto Ragazzoni, Jacopo Farinato, Davide Greggio, Marco Dima, Marco Gullieuszik, et al. "Unmanned aerial vehicles in astronomy." In SPIE Astronomical Telescopes + Instrumentation, edited by Ramón Navarro and James H. Burge. SPIE, 2016. http://dx.doi.org/10.1117/12.2232807.

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Reports on the topic "Instrumentation for Astronomy"

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STUTTGART UNIV (GERMANY F R). Study of Modern Instrumentation and Methods for Astronomic Positioning in the Field. Fort Belvoir, VA: Defense Technical Information Center, March 1988. http://dx.doi.org/10.21236/ada196173.

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