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Titlebook: Exploring the Cosmic Frontier; Astrophysical Instru Andrei P. Lobanov,J. Anton Zensus,Phillip J. Diamo Conference proceedings 2007 Springer

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樓主: 弄混
11#
發(fā)表于 2025-3-23 12:13:02 | 只看該作者
Fizeau Interferometry with the LBT Astronomy on the Way to ELTsbined, focus the LBT provides the spatial resolution of a 23 m telescope and the sensitivity of a 12 m telescope. We are building an instrument called LINC-NIRVANA using the capability of LBT in Fizeau mode (imaging interferometry), leading to a unique combination of spatial resolution, sensitivity
12#
發(fā)表于 2025-3-23 17:48:27 | 只看該作者
MUSE: 3D Spectroscopy with Large Telescopesouthern Observatory (ESO). It is a panoramic integral-field spectrograph operating in the visible wavelength range. It combines a wide field of view with the improved spatial resolution provided by adaptive optics and covers a large simultaneous spectral range. MUSE couples the discovery potential o
13#
發(fā)表于 2025-3-23 18:30:01 | 只看該作者
Layer-Oriented MCAO Projects for 8-m Class Telescopes and Possible Scientific Outcomeod. The purpose of these projects is, in some cases, to give experimental evidence to the Layer-Oriented concept, developed in the last few years. In some other cases, to build real facilities to be used in 8-m class telescopes, like VLT in Chile or LBT in Arizona. A brief description of these proje
14#
發(fā)表于 2025-3-24 00:07:27 | 只看該作者
Prospects for an Extremely Large Synthesis Array). A strawman concept for an Extremely Large Synthesis Array (ELSA) could consist of 27 ten-meter telescopes and baselines of up to 10km [1] (see also Tab. 1). It appears that ELSA could be built today with existing technologies, but the cost would probably be prohibitively high. A technology roadma
15#
發(fā)表于 2025-3-24 04:50:51 | 只看該作者
Interferometry in the Near-Infrared: 1 Mas Resolution at the Wavelength of 1 Micronronomical objects. A large number of key objects have been resolved with unprecedented resolution using bispectrum speckle interferometry or infrared long-baseline interferometry. IR interferometry allows the study of, for example, disks and out- flows of YSOs (e.g., [1]), the wavelength and phase-d
16#
發(fā)表于 2025-3-24 07:36:58 | 只看該作者
17#
發(fā)表于 2025-3-24 14:13:30 | 只看該作者
https://doi.org/10.1007/978-3-540-39756-4Cosmology; Experiment; Gravity; Redshift; SR; STR; Universe; astrophysics
18#
發(fā)表于 2025-3-24 16:34:13 | 只看該作者
19#
發(fā)表于 2025-3-24 22:29:51 | 只看該作者
20#
發(fā)表于 2025-3-25 02:19:37 | 只看該作者
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