Auswahl der wissenschaftlichen Literatur zum Thema „Near Infrared long-Baseline interferometry“
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Zeitschriftenartikel zum Thema "Near Infrared long-Baseline interferometry"
Pan, Xiaopei, Shri Kulkarni, Michael Shao und M. Mark Colavita. „Narrow-Angle and Wide-Angle Astrometry via Long Baseline Optical/Infrared Interferometers“. Symposium - International Astronomical Union 166 (1995): 13–18. http://dx.doi.org/10.1017/s0074180900227769.
Der volle Inhalt der QuelleJankov, S. „Astronomical optical interferometry, II: Astrophysical results“. Serbian Astronomical Journal, Nr. 183 (2011): 1–35. http://dx.doi.org/10.2298/saj1183001j.
Der volle Inhalt der QuelleWittkowski, Markus. „Round Table Summary: Stellar Interferometry as a Tool to Investigate Atmospheres and to Compare Observations with Models“. Symposium - International Astronomical Union 210 (2003): 313–21. http://dx.doi.org/10.1017/s0074180900133455.
Der volle Inhalt der QuelleKraus, S., Th Preibisch und K. Ohnaka. „The inner gaseous accretion disk around a Herbig Be star revealed by near- and mid-infrared spectro-interferometry“. Proceedings of the International Astronomical Union 3, S243 (Mai 2007): 337–44. http://dx.doi.org/10.1017/s1743921307009696.
Der volle Inhalt der QuelleDexter, J. „Event horizon scale emission models for Sagittarius A*“. Proceedings of the International Astronomical Union 9, S303 (Oktober 2013): 298–302. http://dx.doi.org/10.1017/s1743921314000775.
Der volle Inhalt der QuelleCruzalèbes, P., R. G. Petrov, S. Robbe-Dubois, J. Varga, L. Burtscher, F. Allouche, P. Berio et al. „A catalogue of stellar diameters and fluxes for mid-infrared interferometry★“. Monthly Notices of the Royal Astronomical Society 490, Nr. 3 (07.10.2019): 3158–76. http://dx.doi.org/10.1093/mnras/stz2803.
Der volle Inhalt der QuellePetersen, Eric, und Charles Gammie. „Non-thermal models for infrared flares from Sgr A*“. Monthly Notices of the Royal Astronomical Society 494, Nr. 4 (01.05.2020): 5923–35. http://dx.doi.org/10.1093/mnras/staa826.
Der volle Inhalt der QuelleWittkowski, Markus, David A. Boboltz, Malcolm D. Gray, Elizabeth M. L. Humphreys, Iva Karovicova und Michael Scholz. „Radio and IR interferometry of SiO maser stars“. Proceedings of the International Astronomical Union 8, S287 (Januar 2012): 209–16. http://dx.doi.org/10.1017/s1743921312006989.
Der volle Inhalt der QuelleChristou, J. C. „Speckle Interferometry“. Highlights of Astronomy 8 (1989): 561–62. http://dx.doi.org/10.1017/s1539299600008340.
Der volle Inhalt der QuelleChoquet, É., J. Menu, G. Perrin, F. Cassaing, S. Lacour und F. Eisenhauer. „Comparison of fringe-tracking algorithms for single-mode near-infrared long-baseline interferometers“. Astronomy & Astrophysics 569 (September 2014): A2. http://dx.doi.org/10.1051/0004-6361/201220223.
Der volle Inhalt der QuelleDissertationen zum Thema "Near Infrared long-Baseline interferometry"
Ogden, Chad E. „A prototype visible to near-infrared spectrograph for the CHARA array a long-baseline stellar interferometer /“. unrestricted, 2005. http://etd.gsu.edu/theses/available/etd-11282005-121433/.
Der volle Inhalt der QuelleTheo A. ten Brummelaar, committee chair; Brian D. Thoms, Todd J. Henry, William G. Bagnuolo, Douglas R. Gies, Harold A. McAlister, committee members. Author's name from thesis t.p. Electronic text (548 p. : ill.) : digital, PDF file. Description based on contents viewed June 27, 2007; title from title screen. Includes bibliographical references (p. 539-548).
Ogden, Chad Elliott. „A Prototype Visible to Near-Infrared Spectrograph for the CHARA Array, a Long-Baseline Stellar Interferometer“. Digital Archive @ GSU, 2006. http://digitalarchive.gsu.edu/phy_astr_diss/4.
Der volle Inhalt der QuellePourré, Nicolas. „Détection par interférométrie optique d'exoplanètes géantes jeunes à l'échelle de l'unité astronomique“. Electronic Thesis or Diss., Université Grenoble Alpes, 2024. http://www.theses.fr/2024GRALY032.
Der volle Inhalt der QuelleDirect observations provide key information about exoplanetary systems. By analyzing the position of planets at different times, we can determine their orbits and trace the dynamic history of the systems. By analyzing their emission spectra, we can determine the temperature of exoplanets, as well as the chemical composition of their atmosphere, containing tracers of their formation mechanism.However, direct observations are currently limited. Angular resolution limits allow us to observe only the exoplanets furthest from their star, generally more than 10 astronomical units away. Also, the limits of contrast with the host star mean that we can only observe young giant exoplanets, less than 15 Myr, whose infrared thermal radiation is still strong due to their recent formation. To better understand the formation and evolution of planetary systems, these limits must be pushed back to enable direct observations of gas giants on the scale of the astronomical unit.Since 2019, the GRAVITY instrument installed on the Very Large Telescope Interferometer in Chile has made it possible to observe exoplanets at angular separations previously unattainable by conventional direct imaging instruments. Recently, the instrument enabled the first direct observations of the planets β Pictoris c and HD 206893 c, respectively 8.2 and 12.7 masses from Jupiter and 2.7 and 3.5 astronomical units from their star.In summer 2024, the GRAVITY+ upgrade will install new adaptive optics crucial for obtaining better contrast and making observations of less massive exoplanets closer to their star. In 2026, the Gaia space telescope will publish a new list of exoplanets discovered around 2 astronomical units from their star using absolute astrometry. GRAVITY+ will be an instrument of choice for characterizing these planets, measuring their mass and spectrum at wavelengths close to 2 µm.My thesis involves understanding the current limitations of GRAVITY, and preparing the GRAVITY+ upgrade to enable direct observation of "young Jupiters" as close as possible to their star. My thesis was divided into three parts.Firstly, I analyzed data from archival observations to quantify GRAVITY's current limitations in contrast and angular separation. I was able to determine that we could observe exoplanets 30,000 times fainter than their star, down to 50 milli-arcseconds.Secondly, I worked on observational data reduction to understand the source of systematic noise that pollutes exoplanet spectra. I was able to determine the conditions under which these noises appear and their impact on observations.Thirdly, I worked directly on the instrument to implement a high-contrast mode for GRAVITY+. This specific mode for exoplanet observations involves optical aberration correction and wavefront control. The high-contrast mode will limit the impact of host starlight, enabling us to observe less massive and younger exoplanets.In the years to come, the synergy between Gaia and GRAVITY+ will allow us to finely characterize many young giant exoplanets, and certainly transform our vision of how planetary systems form and how they evolve
Grellmann, Rebekka. „Massive star formation as seen by infrared long-baseline interferometry“. Diss., lmu, 2012. http://nbn-resolving.de/urn:nbn:de:bvb:19-149346.
Der volle Inhalt der QuelleGrellmann, Rebekka [Verfasser], und Thomas [Akademischer Betreuer] Preibisch. „Massive star formation as seen by infrared long-baseline interferometry / Rebekka Grellmann. Betreuer: Thomas Preibisch“. München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2012. http://d-nb.info/1027842380/34.
Der volle Inhalt der QuelleMillan-Gabet, Rafael. „Investigation of Herbig Ae /Be stars in the near -infrared with a long baseline interferometer“. 1999. https://scholarworks.umass.edu/dissertations/AAI9950188.
Der volle Inhalt der QuelleBuchteile zum Thema "Near Infrared long-Baseline interferometry"
Danchi, W. C., M. Bester, P. R. McCullough und C. H. Townes. „Infrared Long Baseline Interferometry“. In Highlights of Astronomy, 563–64. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0977-9_89.
Der volle Inhalt der QuelleParesce, F. „Ground-Based Optical/IR Long Baseline Interferometry“. In Infrared Space Interferometry: Astrophysics & the Study of Earth-Like Planets, 85–95. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5468-0_13.
Der volle Inhalt der QuelleKonferenzberichte zum Thema "Near Infrared long-Baseline interferometry"
Rajagopal, Jayadev K., Ryan Lau, Isack Padilla, Stephen T. Ridgway, Choahan Cui, Brittany McClinton, Aqil Sajjad et al. „Towards quantum-enhanced long-baseline optical/near-IR interferometry“. In Optical and Infrared Interferometry and Imaging IX, herausgegeben von Stephanie Sallum, Joel Sanchez-Bermudez und Jens Kammerer, 58. SPIE, 2024. http://dx.doi.org/10.1117/12.3019518.
Der volle Inhalt der QuelleCheriton, Ross, Volodymyr Artyshchuk, Erin Tonita, Glen Herriot, Brent Carlson, Thushara Gunaratne, Zoran Ljusic et al. „Silicon photonic aperture synthesis for long baseline near-infrared interferometry“. In Optical and Infrared Interferometry and Imaging IX, herausgegeben von Stephanie Sallum, Joel Sanchez-Bermudez und Jens Kammerer, 31. SPIE, 2024. http://dx.doi.org/10.1117/12.3019093.
Der volle Inhalt der QuelleKuś, Arkadiusz. „Dual-wavelength, near-infrared holographic tomography“. In Digital Holography and Three-Dimensional Imaging, W4A.33. Washington, D.C.: Optica Publishing Group, 2024. http://dx.doi.org/10.1364/dh.2024.w4a.33.
Der volle Inhalt der QuelleRau, Gioia, Kenneth G. Carpenter, Tabetha Boyajian, Michelle J. Creech-Eakman, Julianne Foster, Margarita Karovska, David Leisawitz et al. „Artemis-enabled stellar imager (AeSI): a Lunar long-baseline UV/optical imaging interferometer“. In Optical and Infrared Interferometry and Imaging IX, herausgegeben von Stephanie Sallum, Joel Sanchez-Bermudez und Jens Kammerer, 54. SPIE, 2024. http://dx.doi.org/10.1117/12.3028797.
Der volle Inhalt der QuelleMerand, Antoine, Pascal Borde und Vincent Coude du Foresto. „A catalog of calibrator stars for 200-meter baseline near-infrared stellar interferometry“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Wesley A. Traub. SPIE, 2004. http://dx.doi.org/10.1117/12.550757.
Der volle Inhalt der QuelleNoecker, M. C., R. W. Babcock, J. D. Phillips und R. D. Reasenberg. „POINTS: technology for micro-arcsecond optical astrometry“. In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1992. http://dx.doi.org/10.1364/oam.1992.fll1.
Der volle Inhalt der QuelleIreland, Michael J., Denis Defrère, Frantz Martinache, John Monnier, Julien Woillez, Peter G. Tuthill und Barnaby Norris. „Image-plane fringe tracker for adaptive-optics assisted long baseline interferometry“. In Optical and Infrared Interferometry and Imaging VI, herausgegeben von Antoine Mérand, Michelle J. Creech-Eakman und Peter G. Tuthill. SPIE, 2018. http://dx.doi.org/10.1117/12.2314393.
Der volle Inhalt der QuelleXu, Teng, Yonghui Hou, Zhongwen Hu, Fanghua Jiang, Zhen Wu, Huimin Kang und Wei Wei. „Development progress of the prototype long baseline optical interferometer in China“. In Optical and Infrared Interferometry and Imaging VII, herausgegeben von Antoine Mérand, Stephanie Sallum und Peter G. Tuthill. SPIE, 2020. http://dx.doi.org/10.1117/12.2562070.
Der volle Inhalt der QuelleHofmann, Karl-Heinz, Matthias Heininger, Dieter Schertl, Gerd Weigelt, Florentin Millour und Philippe Berio. „Image reconstruction method IRBis for optical/infrared long-baseline interferometry“. In SPIE Astronomical Telescopes + Instrumentation, herausgegeben von Fabien Malbet, Michelle J. Creech-Eakman und Peter G. Tuthill. SPIE, 2016. http://dx.doi.org/10.1117/12.2232369.
Der volle Inhalt der QuelleDooley, Jonathan, und Michelle Creech-Eakman. „Initial steps toward a new method of atmospheric characterization over long baseline arrays“. In Optical and Infrared Interferometry and Imaging VI, herausgegeben von Antoine Mérand, Michelle J. Creech-Eakman und Peter G. Tuthill. SPIE, 2018. http://dx.doi.org/10.1117/12.2313853.
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