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Letteratura scientifica selezionata sul tema "Astronomical spectroscopy"

Autore: Grafiati

Pubblicato: 4 giugno 2021

Ultima modifica: 29 luglio 2024

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Articoli di riviste sul tema "Astronomical spectroscopy"

1

Bhattacharyya, J. C. "Astronomical spectroscopy." Resonance 3, no. 5 (May 1998): 24–29. http://dx.doi.org/10.1007/bf02838839.

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Bhattacharyya, J. C. "Astronomical spectroscopy." Resonance 3, no. 6 (June 1998): 16–24. http://dx.doi.org/10.1007/bf02836981.

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3

Miller, David J. "Astronomical spectroscopy: an introduction to the atomic and molecular physics of astronomical spectroscopy." Contemporary Physics 61, no. 4 (October 1, 2020): 304. http://dx.doi.org/10.1080/00107514.2020.1853241.

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4

Panchuk, V. E., M. E. Sachkov, M. V. Yushkin, and M. V. Yakopov. "Integral methods in astronomical spectroscopy." Astrophysical Bulletin 65, no. 1 (January 2010): 75–94. http://dx.doi.org/10.1134/s1990341310010074.

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5

Allamandola, L. J. "Grain Spectroscopy." Symposium - International Astronomical Union 150 (1992): 65–72. http://dx.doi.org/10.1017/s0074180900089725.

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Our fundamental knowledge of interstellar grain composition has grown substantially during the past two decades thanks to significant advances in two areas: astronomical infrared spectroscopy and laboratory astrophysics. The opening of the mid-infrared, the spectral range from 4000-400 cm−1 (2.5-25 μm), to spectroscopic study has been critical to this progress because spectroscopy in this region reveals more about a material's molecular composition and structure than any other physical property.

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Odeh, Mohammad Sh. "Low cost equipment for astronomical spectroscopy." Journal of Instrumentation 16, no. 12 (December 1, 2021): T12009. http://dx.doi.org/10.1088/1748-0221/16/12/t12009.

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Abstract The purpose of this paper is to show how we can obtain spectra for different astronomical objects using low coat equipment. Where a high-efficiency diffraction grating named “The Star Analyzer” was used by the International Astronomical Center (IAC) in Abu Dhabi, UAE to get the spectrum of different astronomical objects. Balmer series was readily visible when observing an “A” type star. TiO absorptions lines were distinguished by observing an “M” type star. Methane absorption lines were visible by observing Uranus and Neptune. Whereas HI and HeI emission lines were detected by observi

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Hentschel, Klaus. "Updating a handbook on astronomical spectroscopy." Journal for the History of Astronomy 46, no. 2 (May 2015): 242–43. http://dx.doi.org/10.1177/0021828614552243.

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Glaspey, John W., and Ian Powell. "A camera for astronomical CCD spectroscopy." Publications of the Astronomical Society of the Pacific 100 (October 1988): 1282. http://dx.doi.org/10.1086/132317.

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DEVORKIN, D. "Astronomical Spectroscopy: The Analysis of Starlight." Science 237, no. 4816 (August 14, 1987): 783–84. http://dx.doi.org/10.1126/science.237.4816.783-a.

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10

Martin-Drumel, M. A., K. L. K. Lee, A. Belloche, O. Zingsheim, S. Thorwirth, H. S. P. Müller, F. Lewen, et al. "Submillimeter spectroscopy and astronomical searches of vinyl mercaptan, C2H3SH." Astronomy & Astrophysics 623 (March 2019): A167. http://dx.doi.org/10.1051/0004-6361/201935032.

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Context. New laboratory investigations of the rotational spectrum of postulated astronomical species are essential to support the assignment and analysis of current astronomical surveys. In particular, considerable interest surrounds sulfur analogs of oxygen-containing interstellar molecules and their isomers. Aims. To enable reliable interstellar searches of vinyl mercaptan, the sulfur-containing analog to the astronomical species vinyl alcohol, we investigated its pure rotational spectrum at millimeter wavelengths. Methods. We extended the pure rotational investigation of the two isomers syn

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Tesi sul tema "Astronomical spectroscopy"

1

Tulloch, Simon. "Astronomical spectroscopy with electron multiplying CCDs." Thesis, University of Sheffield, 2010. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.522382.

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Shaw, Graham David. "New techniques in astronomical multi-slit spectroscopy." Thesis, Durham University, 1993. http://etheses.dur.ac.uk/5643/.

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LDSS-2 is a low dispersion survey spectrograph for the William Herschel Telescope. It was constructed to meet an increasing demand for large scale statistical surveys of stellar and galactic populations. This thesis describes its design, construction and installation, together with additional research concerning the fabrication of multi-slit aperture masks.LDSS-2 has a similar optical system to its predecessor LDSS-1, but it can hold greater numbers of aperture masks, filters and grisms, and its control system is fully automated. This is expected to improve its observing efficiency and allow L

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3

Watson, Frederick Garnett. "Multi-object astronomical spectroscopy with optical fibres." Thesis, University of Edinburgh, 1987. http://hdl.handle.net/1842/27619.

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A full account is given of the relatively new astronomical technique of multi- object spectroscopy with optical fibre lightguides. The thesis begins with a survey of the number densities of a wide range of astronomi- cal object classes, and, after comparing the merits of the various techniques for multi- object spectroscopy, shows (by defining the "effective aperture" of a multiple fibre - coupled telescope) that the multi -fibre tech- nique is very well- suited to the real distribution of celestial objects. A review of the properties of optical fibres is given, together with an exposition of

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4

Haynes, Roger. "Infrared fibres in astronomical instrumentation." Thesis, Durham University, 1995. http://etheses.dur.ac.uk/5402/.

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For several years multi-object spectroscopy systems have been available for carrying out survey work in the visible region, but until very recently there has not been a system for the near infrared region. This thesis describes the design, manufacture and commissioning of the first multi-object fibre system for near infrared spectroscopy. SMIRFS (Spectroscopic Multi-object Infrared Fibre System) is a prototype system that has been designed at the Department of Physics in Durham to couple the Cassegrain focus of the United Kingdom InfraRed Telescope (UKIRT) to a cooled long slit infrared spectr

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5

Porter, Martin John. "A CCD camera system for use in echelle spectroscopy /." St. Lucia, Qld, 2004. http://www.library.uq.edu.au/pdfserve.php?image=thesisabs/absthe17953.pdf.

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Carrasco, Bertha Esperanza. "Further developments of optical fibre techniques for astronomical spectroscopy." Thesis, Durham University, 1992. http://etheses.dur.ac.uk/6029/.

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This thesis describes instrumental techniques pursued to optimise the quality of the spectroscopic data which will be obtained via the new generation of multifibre systems. The technical aspects discussed include the instrumental sources of systematic errors on sky subtraction and new methods to evaluate the fibre performance in terms of throughput and preservation of the input focal ratio. The limiting factor in faint multifibre spectroscopy is the accuracy and reliability of sky subtraction. Instrumentality the precision to which sky subtraction can be done is limited by systematic errors. T

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7

Lee, David. "New techniques in astronomical spectroscopy for 8-m telescopes." Thesis, Durham University, 1998. http://etheses.dur.ac.uk/4847/.

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The purpose of this thesis is to investigate new instrument technology to enhance the capabilities of 8-m telescopes. This thesis first describes the theory, design, construction, and testing of an immersed grating. Immersed gratings can be used to provide R≥ 10(^4) with a multi-object and/or integral field spectrograph on an 8-m telescope. Immersed gratings allow high resolution to be achieved whilst maintaining the required pupil size at a level similar to that on 4-m telescopes. This thesis describes laboratory tests which verify that immersed gratings provide high resolution. The throughpu

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Clampin, Mark. "Investigation of a resistive anode detector for astronomical spectroscopy." Thesis, University of St Andrews, 1986. http://hdl.handle.net/10023/7110.

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A large format two dimensional photon counting detector has been evaluated as a detector for astronomical spectroscopy. The design comprises an 320 photocathode, a tandem MCP gain stage and a circular arc terminated resisitive anode to provide pOSitional coordinates of detected events. The system is run from an LSI 11/23 computer operating under FORTH control. The micro-channel plate operating characteristics and the detector's resolution, quantum efficiency and imaging performance have been studied. The principal areas requiring design improvement are found to be the micro-channel plate gain,

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Oates, Anthony Patrick. "A technique for astronomical spectroscopy with a multi-aperture telescope." Thesis, University of Central Lancashire, 1985. http://clok.uclan.ac.uk/19078/.

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A technique for acquiring spectral line data using a multi-aperture telescope is described. The multi-aperture principle and the criteria which led to the selection of a dispersive spectrometer are discussed. The problem of linking telescope and spectrometer has been solved by incorporating low loss optical fibres and this is also discussed. The problems of automatic data collection, its manipulation, display and storage presented a major research effort which were largely overcome by the use of cheap, digital micro-computers. To achieve rapid and flexible data handling the i.E.E.E. bus was us

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Bounissou, Sophie. "”On-chip” astronomical instrumentation : bringing polarimetric and spectroscopic capabilities to the detector level." Thesis, Université Paris-Saclay (ComUE), 2019. http://www.theses.fr/2019SACLS400.

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Cette thèse étudie la possibilité d'intégrer plusieurs fonctions instrumentales au sein de la matrice de bolomètres pour les observations dans le domaine du sub-millimétrique. Ceci est désormais envisageable grâce aux progrès des micro-technologies.Dans un premier temps, nous avons optimisé le design des pixels polarimétriques inventés pour l'instrument B-BOP du futur observatoire spatial SPICA. Ce travail a notamment permis de quantifier la cross-polarisation (1/1000) et de repenser la géométrie des pixels afin d'obtenir des détecteurs mieux adaptés au rayonnement incident.Cette thèse a égale

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Libri sul tema "Astronomical spectroscopy"

1

Kitchin, C. R. Optical astronomical spectroscopy. Bristol: Institute of Physics Pub., 1995.

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2

Harrison, Ken M. Astronomical Spectroscopy for Amateurs. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-7239-2.

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3

David, Emerson. Interpreting astronomical spectra. Chichester: J. Wiley & Sons, 1996.

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4

Hadrava, Petr. Stellar spectroscopy at Ondřejov Observatory. Ondřejov: Astronomical Institute of the Academy of Sciences of the Czech Republic, 2004.

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5

S, Kwok, ed. Astronomical infrared spectroscopy: Future observational directions. San Francisco, Calif: Astronomical Society of the Pacific, 1993.

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6

Derviz, T. E. Astronomicheskie spektrografy: Uchebnoe posobie. Leningrad: Leningradskiĭ universitet, 1985.

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7

D, Garmany C., Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder. Dept. of Astrophysical, Planetary, and Atmospheric Sciences, and United States. National Aeronautics and Space Administration, eds. Spectroscopic observations of selected stellar systems. Boulder, Colo: Joint Institute for Laboratory Astrophysics, 1985.

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8

Torres, Rafael Escribano. Spectroscopy of the atmospheres. Madrid: Consejo Superior de Investigaciones Científicas, 2010.

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A, Dalgarno, and Layzer David, eds. Spectroscopy of astrophysical plasmas. Cambridge, CB: Cambridge University Press, 1987.

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10

Observatory, Anglo-Australian, ed. The UCL Echelle spectograph. Epping, N.S.W: Anglo-Australian Observatory, Epping Laboratory, 1989.

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Capitoli di libri sul tema "Astronomical spectroscopy"

1

Lawrence, Andy. "Spectroscopy." In Astronomical Measurement, 121–44. Berlin, Heidelberg: Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-39835-3_5.

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2

Massey, Philip, and Margaret M. Hanson. "Astronomical Spectroscopy." In Planets, Stars and Stellar Systems, 35–98. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-5618-2_2.

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3

Ade, Peter A. R., Griffin Matthew J., and Carole E. Tucker. "Astronomical Spectroscopy." In Physical Principles of Astronomical Instrumentation, 123–54. Boca Raton: CRC Press, 2021. http://dx.doi.org/10.1201/9781315374659-7.

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Schmidt, Timothy W. "Astronomical Molecular Spectroscopy." In Computational Spectroscopy, 377–98. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2010. http://dx.doi.org/10.1002/9783527633272.ch13.

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Mertz, Lawrence. "Spectroscopy." In Excursions in Astronomical Optics, 95–107. New York, NY: Springer New York, 1996. http://dx.doi.org/10.1007/978-1-4612-2386-3_5.

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Hopkins, Jeffrey L. "Amateur Astronomical Spectroscopy." In The Patrick Moore Practical Astronomy Series, 45–73. Cham: Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01442-5_2.

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Hopkins, Jeffrey L. "Astronomical Spectroscopy Projects." In The Patrick Moore Practical Astronomy Series, 233–51. Cham: Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01442-5_8.

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Harrison, Ken M. "A History of Astronomical Spectroscopy." In Patrick Moore's Practical Astronomy Series, 9–14. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7239-2_2.

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Escribano, Rafael, and Guillermo M. Muñoz Caro. "Introduction to Spectroscopy and Astronomical Observations." In Laboratory Astrophysics, 27–47. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-90020-9_3.

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Maillard, J. P. "Astronomical Fourier-Transform Spectroscopy of the 1990s." In Progress in Fourier Transform Spectroscopy, 133–41. Vienna: Springer Vienna, 1997. http://dx.doi.org/10.1007/978-3-7091-6840-0_16.

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Atti di convegni sul tema "Astronomical spectroscopy"

1

HOLT, STEPHEN S. "X-RAY ASTRONOMICAL SPECTROSCOPY." In A Festschrift in Honor of Ricardo Giacconi. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812792174_0006.

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2

Serabyn, E., and E. Weisstein. "Submillimeter Fourier Transform Spectroscopy of Astronomical Sources." In Fourier Transform Spectroscopy. Washington, D.C.: Optica Publishing Group, 1995. http://dx.doi.org/10.1364/fts.1995.ffd14.

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From the 4000 m altitude of Mauna Kea, submillimeter wavelength astronomical observations are often possible at frequencies up to nearly 1 THz. To measure broadband astronomical and atmospheric spectra in the available atmospheric transmission windows between 150 GHz and 1 THz, we have built a moderate resolution (λ/Δλ < 5000) Fourier Transform Spectrometer for use at the Caltech Submillimeter Observatory (CSO). The instrument is a dielectric-beamsplitter rapid-scan FTS which uses the CSO’s facility bolometer as its single detecting element. Five bandpass filters are used to match to the av

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3

Dallier, Richard, and Jean Gabriel Cuby. "Noncooled near-infrared spectroscopy." In Astronomical Telescopes & Instrumentation, edited by Albert M. Fowler. SPIE, 1998. http://dx.doi.org/10.1117/12.317246.

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Serabyn, Eugene. "Submillimeter Fourier transform spectroscopy." In Astronomical Telescopes & Instrumentation, edited by Thomas G. Phillips. SPIE, 1998. http://dx.doi.org/10.1117/12.317347.

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Serabyn, E., and J. R. Pardo. "Astronomical and Atmospheric Fourier Transform Spectroscopy at Submillimeter Wavelengths." In Fourier Transform Spectroscopy. Washington, D.C.: OSA, 2001. http://dx.doi.org/10.1364/fts.2001.fmb1.

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Naylor, D. A., and B. G. Gom. "FTS-2: A Submillimetre Astronomical Imaging Fourier Transform Spectrometer." In Fourier Transform Spectroscopy. Washington, D.C.: OSA, 2007. http://dx.doi.org/10.1364/fts.2007.fwa1.

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7

Stern, R. A., R. C. Catura, M. M. Blouke, and M. Winzenread. "EUV Astronomical Spectroscopy With CCD Detectors." In 1986 Astronomy Conferences, edited by David L. Crawford. SPIE, 1986. http://dx.doi.org/10.1117/12.968135.

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8

Joyce, Richard R., Kenneth H. Hinkle, Michael R. Meyer, and Michael F. Skrutskie. "Infrared astronomical spectroscopy with a noncryogenic spectrograph." In Astronomical Telescopes & Instrumentation, edited by Albert M. Fowler. SPIE, 1998. http://dx.doi.org/10.1117/12.317339.

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Burgarella, Denis, Kjetil Dohlen, Veronique Buat, Gerard R. Lemaitre, and Annie Perez. "Multi-object spectroscopy in space." In Astronomical Telescopes & Instrumentation, edited by Pierre Y. Bely and James B. Breckinridge. SPIE, 1998. http://dx.doi.org/10.1117/12.324436.

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Smith, Erin C., and Ian S. McLean. "Grism spectroscopy with FLITECAM." In SPIE Astronomical Telescopes + Instrumentation, edited by Ian S. McLean and Masanori Iye. SPIE, 2006. http://dx.doi.org/10.1117/12.672174.

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