Gotowe bibliografie tematyczne / Telescope Infrared

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Gotowa bibliografia na temat „Telescope Infrared”

Autor: Grafiati

Data publikacji: 3 czerwca 2025

Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Telescope Infrared"

Burton, Michael G., John W. V. Storey, and Michael C. B. Ashley. "Science Goals for Antarctic Infrared Telescopes." Publications of the Astronomical Society of Australia 18, no. 2 (2001): 158–65. http://dx.doi.org/10.1071/as01026.

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AbstractOver the past few years, site-testing at the South Pole has revealed conditions that are uniquely favourable for infrared astronomy. In particular, the exceptionally low sky brightness throughout the near and mid-infrared leads to the possibility of a modest-sized telescope achieving comparable sensitivity to that of existing 8–10 metre class telescopes. An 8 metre Antarctic telescope, if constructed, would yield performance that would be unrivalled until the advent of the NGST. In this paper we review the scientific potential of infrared telescopes in Antarctica, and discuss their com

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Wang, Jing-Sheng. "Newly Installed Radio and Optical Telescopes in China." Publications of the Astronomical Society of Australia 9, no. 1 (1991): 60–61. http://dx.doi.org/10.1017/s1323358000024899.

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AbstractNew radio and optical telescopes installed in recent years in China are summarised. These include the 2.16-m optical telescope, the solar magnetic field telescope, the Miyun synthesis radio telescope, the 1.26-m infrared telescope (Beijing Astronomical Observatory), the 25-m radio telescope as the first station of China’s VLBI network, the 1.56-m astrometric telescope (Shanghai Observatory), and the 13.7-m millimetre wave radio telescope.

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Liu, Xuan, Junhong Deng, King Fai Li, et al. "Optical telescope with Cassegrain metasurfaces." Nanophotonics 9, no. 10 (2020): 3263–69. http://dx.doi.org/10.1515/nanoph-2020-0012.

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AbstractThe Cassegrain telescope, made of a concave primary mirror and a convex secondary mirror, is widely utilized for modern astronomical observation. However, the existence of curved mirrors inevitably results in bulky configurations. Here, we propose a new design of the miniaturized Cassegrain telescope by replacing the curved mirrors with planar reflective metasurfaces. The focusing and imaging properties of the Cassegrain metasurface telescopes are experimentally verified for circularly polarized incident light at near infrared wavelengths. The concept of the metasurface telescopes can

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Werner, M. W., William T. Reach, and M. Rieke. "Studies of the Cosmic Infrared Background with the Space Infrared Telescope Facility (SIRTF)." Symposium - International Astronomical Union 204 (2001): 439–53. http://dx.doi.org/10.1017/s0074180900226405.

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IRAS, COBE, and ISO have demonstrated the unique importance of a cryogenic infrared telescope in space for studying diffuse infrared backgrounds and for teasing out the individual point sources which contribute to them. This importance results from the extremely high infrared sensitivity of such telescopes, particularly to diffuse radiation. The next cryogenic infrared telescope will be NASA's Space Infrared Telescope Facility (SIRTF), which is currently in the final stages of construction leading to launch in 2002. SIRTF will be the first infrared space observatory to make extensive use - bot

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Kim, Daewook, Youngsik Kim, Heejoo Choi, Yuzuru Takashima, and Christopher Walker. "Inflatable On-Axis and Off-Axis Space Telescope Designs." EPJ Web of Conferences 309 (2024): 03001. http://dx.doi.org/10.1051/epjconf/202430903001.

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In the realm of astronomical scientific exploration, deployable and scalable approaches in space telescope systems are reshaping our understanding of the universe. Two revolutionary membrane-based space telescope designs, on-axis OASIS (Orbiting Astronomical Satellite for Investigating Stellar Systems) and off-axis SALTUS (Single Aperture Large Telescope for Universe Studies), have been developed as mid/far-infrared telescope concepts featuring an inflatable primary mirror. Through the scalable primary aperture design, these deployable space telescopes leverage an all-encompassing optical arch

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Persi, P., A. Preite-Martinez, and M. Ferrari-Toniolo. "Infrared Energy Distribution of Selected Planetary Nebulae." Symposium - International Astronomical Union 131 (1989): 57. http://dx.doi.org/10.1017/s007418090013757x.

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Caicoya, P. G. R., M. B. Cabrera, P. F. Izquierdo, J. Patrón, V. Sánchez De La Rosa, and F. T. Sangines. "From 1.5 Meters to 10.4 Meters in 20 Years: Technological Evolution at the Instituto de Astrofísica de Canarias in the Development of Infrared Instrumentation for Terrestrial Telescopes." Journal of Astronomical Instrumentation 03, no. 03n04 (2014): 1450005. http://dx.doi.org/10.1142/s2251171714500056.

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This paper reviews the evolution of the technical development of infrared instrumentation for terrestrial telescopes at the Instituto de Astrofísica de Canarias (IAC). The three most representative instruments, CAIN (installed on the 1.5 m Carlos Sánchez Telescope), LIRIS (on the 4.2 m William Herschel Telescope), and EMIR (on the 10.4 m Gran Telescopio Canarias) are described and compared. Each project entailed an improvement and a technological advance in relation to its predecessor. Larger optical beams brought larger lenses, larger mechanisms to hold them, stiffer and more massive support

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Torres-Quijano, Amílcar R., Christopher Packham, and Sergio Fernandez Acosta. "CanariCam Mid-infrared Drift Scanning: Improved Sensitivity and Spatial Resolution." Publications of the Astronomical Society of the Pacific 133, no. 1029 (2021): 114501. http://dx.doi.org/10.1088/1538-3873/ac2ec3.

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Abstract Ground-based mid-infrared (MIR) astronomical observations require the removal of the fast time variable components of (a) sky/background variation and (b) array background. Typically, this has been achieved through oscillating the telescope’s secondary mirror a few times a second, a process termed “chopping.” However, chopping reduces on-object photon collection time, imposes stringent demands on the secondary mirror, requires nodding of the telescope to remove the radiative offset imprinted by the chopping, and relies on an often-fixed chop-frequency regardless of the sky conditions

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Song, Su. "Evolutions and Principles of Space and Radio Telescope." Highlights in Science, Engineering and Technology 72 (December 15, 2023): 47–52. http://dx.doi.org/10.54097/8r8fyx84.

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Contemporarily, various types of telescopes have been proposed as tools for cosmology observation. This study discusses main types of telescopes, i.e., space and radio telescopes people used to observe universe and gives deep description and comparison between them. Radio telescope is the telescope which can receive radio waves from the outer space and can detect waves in different wavelengths besides visible light. It has a long history, as radio telescope is built on Earth and relatively easier for people to make it, but the drawback is that radio telescope may be disturbed by nature conditi

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Kim, Dae Wook, Christopher K. Walker, Dániel Apai, et al. "Disruptive space telescope concepts, designs, and developments: OASIS and Nautilus -INVITED." EPJ Web of Conferences 238 (2020): 06001. http://dx.doi.org/10.1051/epjconf/202023806001.

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Two disruptive space telescope concepts are being designed and developed at the University of Arizona; these are the 20-meter OASIS (Orbiting Astronomical Satellite for Investigating Stellar Systems) and 8.5-meter Nautilus. OASIS combines break-through inflatable aperture and adaptive optics techniques to realize the dream of a 20+ meter class spaceborne terahertz/far-infrared telescope. In the Nautilus visible/near-infrared telescope concept, conventional primary mirrors are replaced by an ~8.5-meter MODE (Multi-order diffractive engineered) lens with 10 times lower areal density and up to 10

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Rozprawy doktorskie na temat "Telescope Infrared"

Querel, Richard Robert, and University of Lethbridge Faculty of Arts and Science. "IRMA calibrations and data analysis for telescope site selection." Thesis, Lethbridge, Alta. : University of Lethbridge, Faculty of Arts and Science, 2007, 2007. http://hdl.handle.net/10133/675.

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Our group has developed a 20 μm passive atmospheric water vapour monitor. The Infrared Radiometer for Millimetre Astronomy (IRMA) has been commissioned and deployed for site testing for the Thirty Meter Telescope (TMT) and the Giant Magellan Telescope (GMT). Measuring precipitable water vapour (PWV) requires both a sophisticated atmospheric model (BTRAM) and an instrument (IRMA). Atmospheric models depend on atmospheric profiles. Most profiles are generic in nature, representing only a latitude in some cases. Site-specific atmospheric profiles are required to accurately simulate the atmosphere

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O'Donnell, D. V. (Daniel V. ). 1983. "An infrared survey of galaxy clusters with the Spitzer Space Telescope /." Thesis, McGill University, 2008. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=111564.

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We present the observations, reduction and preliminary analysis of a sample of 45 mid-to-high redshift galaxy clusters imaged with the Spitzer Space Telescope's MIPS camera at 24 ~m and selected from the Red Sequence Cluster Survey. The purpose of the data set is motivated by a broad review of studies into the evolutionary trends of galaxy clusters and their constituent galaxy populations, focusing specifically on recent results that indicate clusters are environmental drivers of dusty starburst and active galactic nuclei activity. To accommodate the large amount of data in hand, we have const

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Spalding, Eckhart, Andrew Skemer, Philip M. Hinz, and John M. Hill. "Infrared photometry with 'wall-eyed' pointing at the Large Binocular Telescope." SPIE-INT SOC OPTICAL ENGINEERING, 2016. http://hdl.handle.net/10150/622809.

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The brightness and variability of the atmosphere in the thermal infrared poses obstacles to precision photometry measurements. The need to remove atmospheric effects calls for the use of a comparison star, but it is usually impossible to fit both science and comparison targets on current long-wavelength (> 2 mu m) detectors. We present a new pointing mode at the Large Binocular Telescope, which has twin 8.4-m primary mirrors that can be pointed up to similar to 2 arcminutes apart and allow the placement of both targets on a small-field infrared detector. We present an observation of the primar

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Lenssen, Nathan. "Fundamental Limits of Detection in the Near and Mid Infrared." Scholarship @ Claremont, 2013. http://scholarship.claremont.edu/cmc_theses/800.

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The construction of the James Webb Space Telescope has brought attention to infrared astronomy and cosmology. The potential information about our universe to be gained by this mission and future infrared telescopes is staggering, but infrared observation faces many obstacles. These telescopes face large amounts of noise by many phenomena, from emission off of the mirrors to the cosmic infrared background. Infrared telescopes need to be designed in such a way that noise is minimized to achieve sufficient signal to noise ratio on high redshift objects. We will investigate current and planned spa

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Tansley, David. "ISO observations of dust in low redshift radio galaxies." Thesis, University of Bristol, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.324359.

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Magdis, Georgios E. "Mid-Infrared Studies of Lyman Break Galaxies with the Spitzer Space Telescope." Thesis, University of Oxford, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.514965.

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Ramphul, Rajin Anand. "Characterising star forming and luminous infrared galaxies with the Southern African Large Telescope (SALT)." Thesis, University of Cape Town, 2018. http://hdl.handle.net/11427/28380.

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Context: Stellar population modelling is a popular technique that has been extensively applied to main sequence galaxies. Yet starburst galaxies and Luminous InfraRed Galaxies (LIRGs) have, so far, not been studied as much using the method. LIRGs in the local universe are known to be highly interacting galaxies with strong star formation in obscured environments. Still, LIRGs also have diversity in terms of morphology and mode and location of star formation. Aim: This thesis investigates the stellar population properties of a group of 52 starbursts and luminous infrared galaxies (LIRGs) in the

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Greene, Thomas P., Douglas M. Kelly, John Stansberry та ін. "λ = 2.4 to 5 μm spectroscopy with the James Webb Space Telescope NIRCam instrument". SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS, 2017. http://hdl.handle.net/10150/626090.

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The James Webb Space Telescope near-infrared camera (JWST NIRCam) has two 2.'2 x 2.'2 fields of view that can be observed with either imaging or spectroscopic modes. Either of two R similar to 1500 grisms with orthogonal dispersion directions can be used for slitless spectroscopy over lambda = 2.4 to 5.0 mu m in each module, and shorter wavelength observations of the same fields can be obtained simultaneously. We describe the design drivers and parameters of the grisms and present the latest predicted spectroscopic sensitivities, saturation limits, resolving powers, and wavelength coverage val

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Lowe, Krispian Tom Edward. "Infrared polarimetry and integral field spectroscopy of post-asymptotic giant branch stars." Thesis, University of Hertfordshire, 2008. http://hdl.handle.net/2299/2449.

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In this thesis, I present the properties of IRAS 19306+1407 central source and its sur- rounding circumstellar envelope (CSE), from the analysis of near-infrared (near-IR) polarimetry and integral field spectroscopy (IFS), with supporting archived HST im- ages and sub-millimetre (sub-mm) photometry. This is supported by axi-symmetric light scattering (ALS), axi-symmetric radiative transfer (DART) and molecular hy-drogen (H2) shock models. The polarimetric images show that IRAS 19306+1407 has a dusty torus, which deviates from axisymmetry and exhibits a ‘twist’ feature. The DART and ALS modelli

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Gaspar, Andras. "Observations and Models of Infrared Debris Disk Signatures and their Evolution." Diss., The University of Arizona, 2011. http://hdl.handle.net/10150/202982.

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In my thesis I investigate the occurrence of mid-infrared excess around stars and their evolution. Since the launch of the first infrared satellite, IRAS, we have known that a large fraction of stars exhibit significant levels of infrared emission above their predicted photospheric level. Resolved optical and infrared images have revealed the majority of these excesses to arise from circumstellar disk structures, made up of distributions of planetesimals, rocks, and dust. These structures are descriptively called debris disks. The first part of my thesis analyzes the Spitzer Space Telescope Ob

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Książki na temat "Telescope Infrared"

J, Irvine Nelson, and United States. National Aeronautics and Space Administration., eds. SIRTF, Space Infrared Telescope Facility: A window on cosmic birth. National Aeronautics and Space Administration, 1990.

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Powell, J. David. Space infrared telescope pointing control system: Infrared telescope tracking in the presence of target motion : final report. Guidance and Control Laboratory, Dept. of Aeronautics and Astronautics, Stanford University, 1986.

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Davies, John K. The Life Story of an Infrared Telescope. Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-23579-0.

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Fazio, Giovanni G. A balloon-borne 102-cm telescope for far-infrared astronomy. Smithsonian Astrophysical Observatory, 1990.

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Fazio, Giovanni G. A balloon-borne 102-cm telescope for far-infrared astronomy. Smithsonian Astrophysical Observatory, 1990.

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United States. National Aeronautics and Space Administration., ed. Space infrared telescope facility project: Final technical report. National Aeronautics and Space Administration, 1988.

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Fazio, Giovanni G. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy. Smithsonian Institution, Astrophysical Observatory, 1986.

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Fazio, Giovanni G. Balloon-borne three-meter telescope for far-infrared and submillimeter astronomy. Smithsonian Institution, Astrophysical Observatory, 1986.

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Powell, J. David. Space infrared telescope pointing control system: Automated star pattern recognition : final report. National Aeronautics and Space Administration, 1985.

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Rottner, Renee M. Making the invisible visible: A history of the Spitzer Infrared Telescope Facility (1971-2003). National Aeronautics and Space Administration, NASA History Program Office, 2012.

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Części książek na temat "Telescope Infrared"

Nishimura, Tetsuo. "Infrared Detector For Mid-Infrared Astronomy." In Japanese National Large Telescope and Related Engineering Developments. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-017-2003-8_40.

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Erickson, E. F., and M. W. Werner. "SIRTF: Space Infrared Telescope Facility." In Next Generation Infrared Space Observatory. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2680-9_9.

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Matsumoto, T. "Infrared Telescope in Space: IRTS." In Infrared and Submillimeter Space Missions in the Coming Decade. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0363-3_9.

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Matsumoto, Toshio. "IRTS: Infrared Telescope in Space." In Observatories in Earth Orbit and Beyond. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-011-3454-5_24.

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Livingston, W. "A 4-meter McMath Telescope for the Infrared." In Infrared Solar Physics. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1926-9_70.

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Fazio, Giovanni G., and Peter Eisenhardt. "The Space Infrared Telescope Facility (SIRTF)." In Observatories in Earth Orbit and Beyond. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-011-3454-5_22.

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Bock, James J., Andrew E. Lange, T. Matsumoto, Peter B. Eisenhardt, Perry B. Hacking, and Helene R. Schember. "NIFTE: The near Infrared Faint-Object Telescope Experiment." In Infrared Astronomy with Arrays. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1070-9_83.

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Bely, Pierre Y., Holland C. Ford, Richard Burg, Larry Petro, Rick White, and John Bally. "POST: Polar Stratospheric Telescope." In Infrared and Submillimeter Space Missions in the Coming Decade. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0363-3_13.

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Maihara, Toshinori. "Infrared Instruments For JNLT." In Japanese National Large Telescope and Related Engineering Developments. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-017-2003-8_39.

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Matthews, K., and B. T. Soifer. "The Near Infrared Camera on the W.M. Keck Telescope." In Infrared Astronomy with Arrays. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1070-9_76.

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Streszczenia konferencji na temat "Telescope Infrared"

van Belle, Gerard T., and Anders M. Jorgensen. "The Big Fringe Telescope." In Optical and Infrared Interferometry and Imaging IX, edited by Stephanie Sallum, Joel Sanchez-Bermudez, and Jens Kammerer. SPIE, 2024. http://dx.doi.org/10.1117/12.3020515.

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Baryshev, Andrey M., Martina C. Wiedner, Paul K. Grimes, Ron J. Vervack, Asantha Cooray, and Meredith MacGregor. "FIRSST : Far-Infrared Spectroscopy Space Telescope." In Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII, edited by Jonas Zmuidzinas and Jian-Rong Gao. SPIE, 2024. http://dx.doi.org/10.1117/12.3020666.

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Cooray, Asantha, Meredith MacGregor, Ronald J. Vervack, et al. "Far-infrared spectroscopy space telescope (FIRSST)." In Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave, edited by Laura E. Coyle, Marshall D. Perrin, and Shuji Matsuura. SPIE, 2024. http://dx.doi.org/10.1117/12.3019435.

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Köhler, Rainer, Edgar R. Ligon, Matthew D. Anderson, et al. "Integrating a mobile telescope into the CHARA array." In Optical and Infrared Interferometry and Imaging IX, edited by Stephanie Sallum, Joel Sanchez-Bermudez, and Jens Kammerer. SPIE, 2024. http://dx.doi.org/10.1117/12.3020620.

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Schember, Helene R., Paul K. Manhart, Cecilia N. Guiar, and James H. Stevens. "Space Infrared Telescope Facility telescope overview." In San Diego, '91, San Diego, CA, edited by Bjorn F. Andresen, Marija Scholl, and Irving J. Spiro. SPIE, 1991. http://dx.doi.org/10.1117/12.48714.

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Kim, Daewook, Jonathan W. Arenberg, Yuzuru Takashima, Art Palisoc, and Christopher Walker. "SALTUS Probe Class Space Mission: Enabled by 20-m Inflatable Mirror." In CLEO: Applications and Technology. Optica Publishing Group, 2022. http://dx.doi.org/10.1364/cleo_at.2022.aw4i.2.

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SALTUS (Single Aperture Large Telescope for Universe Studies) is a mid/far-infrared telescope concept utilizing a 20-m scale inflatable mirror antenna. The light-weight mirror utilizes a membrane architecture that has been developed and characterized specifically for space-based applications. The telescope's end-to-end optical design and optimization process unleashes the unprecedented photon collecting power of a large space aperture. A series of inflatable mirror prototypes have been designed, manufactured, and tested. These tests confirmed the optical performance of the apertures under spac

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Johnson, R. Barry. "Very-broad spectrum afocal telescope." In International Optical Design Conference. Optica Publishing Group, 1998. http://dx.doi.org/10.1364/iodc.1998.lfa.4.

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The design of high-magnification afocal telescopes that operate simultaneously over very-broad portions of the visible and infrared spectrums presents a significant challenge to the lens designer.1 Such telescopes are often used with some type of scanning sensor that requires the pupil of the telescope to be located external to the telescope to afford alignment with the sensor’s pupil. The afocal telescope described in this paper comprises a single primary mirror and two lenses to form the secondary optics where each lens is made from the same material. The secondary spectrum of the telescope

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Beckers, Jacques M. "The National New Technology Telescope as a phased array." In OSA Annual Meeting. Optica Publishing Group, 1986. http://dx.doi.org/10.1364/oam.1986.ma1.

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The National New Technology Telescope (NNTT) is a monolithic array of four 7.5-m diam telescopes which has a light-gathering power equivalent to that of a 15-m single-mirror telescope and an angular resolution, when phased, equivalent to a 21-m single-mirror telescope. I describe the telescope, its astronomical capabilities, the techniques which will be used to both coalign and cophase the array and to give a large phased field of view, and the plans to obtain diffraction-limited imaging at optical and infrared wavelengths. The design of the NNTT is based on the experience gained with the six-

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Merkle, Fritz. "Interferometry with the European Very Large Telescope." In OSA Annual Meeting. Optica Publishing Group, 1986. http://dx.doi.org/10.1364/oam.1986.ma3.

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In the present Very Large Telescope (VLT) linear array concept four independent telescopes of the 8-m class are coupled together. This offers the unique possibility to operate the telescopes as an optical and/or infrared long base-line interferometer. The first target for an interferometric operation is the infrared range from 5 to 20 μm and later a gradual expansion to shorter wavelengths. In the interferometric mode the gain of the 8-m diam single apertures of the VLT is only given, if adaptive optics is used for a real-time partial or full phase compensation of the degradations due to atmos

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Norris, David, Mary Bothwell, and Joseph Plamondon. "Space Infrared Telescope Facility." In Space Optics for Astrophysics and Earth and Planetary Remote Sensing. Optica Publishing Group, 1991. http://dx.doi.org/10.1364/soa.1991.tub1.

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The Space Infrared Telescope Facility (SIRTF) is the fourth and last Great Observatory of the NASA Astrophysics Program. The challenges in providing this Observatory range from new cryogenic optical and sensing technology to operating in a fixed price research environment.

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Raporty organizacyjne na temat "Telescope Infrared"

Goode, Philip R. First Light Infrared Observations with the 1.6 Meter Solar Telescope in Big Bear: Origins of Space Weather Telescope. Defense Technical Information Center, 2012. http://dx.doi.org/10.21236/ada577214.

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Goode, Philip. Infrared Observations with the 1.6 Meter New Solar Telescope in Big Bear: Origins of Space Weather. Defense Technical Information Center, 2015. http://dx.doi.org/10.21236/ada619946.

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