... Adaptive Optics Systems, Optical Interferometry Systems and Wavefront sensing ... C. Straubmeier, S. Rost, Y. Wang, A. Eckart, in Advances in Stellar Interferometry ... C. Arcidiacono, in Optical and Infrared Interferometry, Editors M. SchЖller, W. C ...
... I. 1997, Nature 388, 555 Sargent A.I. & Beckwith S.V.W. 1994, in IAU Coll. n. 140, Astronomy with Millimeter and Submillimeter Wave Interferometry, ed. M. Ishiguro & W.J. Welch (San Francisco: ASP), 203 Shu F.H., Najita J.R., Shang H., Li, Z.-Y. 2000, in ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/dgtau/dgtau.ps.gz -- 157.0 Кб -- 11.09.2007 Похожие документы
... Millimeter wavelength interferometry o ers both a high spatial resolution and high sensi- tivity that are critical to shredding light on this problem. ...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/imaging99/tuc.ps.gz -- 390.4 Кб -- 11.09.2007 Похожие документы
... Millimeter wavelength interferometry offers both a high spatial resolution and high sensitivity that are critical to shredding light on this problem. ...
... In order to simplify the interface between OPM and SPG (only one beams triplet at the entrance of the spectrograph) the separation between photometry and interferometry channels is inserted into the spectrograph cryostat, just before the grating. ...
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Ссылки http://www.arcetri.astro.it/irlab/instr/amber/docs/llsspe.pdf -- 129.2 Кб -- 23.09.2006 Похожие документы
... the future telescope in Greenland (hence the name Greenland Telescope), the Submillimeter Array in Hawaii, and the Atacama Large Millimeter/submillimeter Array in Chile, will play a key role for future Very Long Baseline Interferometry (VLBI) observation ...
... Genzel, R., Baker, A.J., Tacconi, L.J., Lutz, D., Cox, P.; Guilloteau, S., Omont, A. Spatially Resolved Millimeter Interferometry of SMM J02399-0136: A Very Massive Galaxy at z = 2.8. ...
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Ссылки http://www.arcetri.astro.it/science/k20/papers/og_final.pdf -- 264.2 Кб -- 30.11.2004 Похожие документы
... LBT primary) The 2.1 m adaptive secondary is made by 7(LBT secondary) segments Priority on IR interferometry (exoplanets) ·Primary: 7 large active segments ·Adaptive optics: -Segmented Adaptive Secondary -Further TBD correctors in beam combiner Munich Dec ...
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Ссылки http://www.arcetri.astro.it/~salinari/GSF/Wavefront%20Control.pdf -- 1770.4 Кб -- 27.11.2003 Похожие документы