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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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书目名称Exploring the Cosmic Frontier
副标题Astrophysical Instru
编辑Andrei P. Lobanov,J. Anton Zensus,Phillip J. Diamo
视频video
丛书名称ESO Astrophysics Symposia
图书封面Titlebook: Exploring the Cosmic Frontier; Astrophysical Instru Andrei P. Lobanov,J. Anton Zensus,Phillip J. Diamo Conference proceedings 2007 Springer
描述.In the coming decades, astrophysical science will benefit enormously from the construction and operation of several major international ground- and space based facilities, such as ALMA, Herschel/Planck, and SKA in the far infrared to radio band, Extremely Large Telescopes, JWST and GAIA in the optical to near infrared regime, XEUS and Constellation-X in the X-ray, and GLAST in the Gamma-ray regime. These and other new instruments will have a major impact in a wide range of scientific topics including the cosmological epoch of reionization, galactic dynamics and nuclear activity, stellar astronomy, extra-solar planets, gamma-ray bursts, X-ray binaries, and many others...On May 18-21, 2004, the Max-Planck-Society’s Harnack-Haus in Dahlem, Berlin hosted the international symposium "Exploring the Cosmic Frontier: Astrophysical Instruments for the 21st Century". The symposium in Berlin was dedicated to exploring the complementarity and synergies between different branches of astrophysical research, by presenting and discussing the fundamental scientific problems that will be addressed by major future astrophysical facilities in the next few decades...This book contains 70 papers from t
出版日期Conference proceedings 2007
关键词Cosmology; Experiment; Gravity; Redshift; SR; STR; Universe; astrophysics
版次1
doihttps://doi.org/10.1007/978-3-540-39756-4
isbn_softcover978-3-642-07259-8
isbn_ebook978-3-540-39756-4Series ISSN 1431-2433 Series E-ISSN 1611-6143
issn_series 1431-2433
copyrightSpringer-Verlag Berlin Heidelberg 2007
The information of publication is updating

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Design of the Near-term Next Generation Space-VLBI Mission VSOP-2esolution imaging of astrophysically exotic regions, including the cores, jets, and accretion disks of active galactic nuclei (AGN), water maser emissions, micro-quasars, coronae of young stellar objects, etc. A highest angular resolution of about 40 .as is achieved in the 43 GHz band. Engineering d
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Imaging Across the Spectrum: Synergies Between SKA and Other Future Telescopessynergies in astrophysical research made across different spectral bands presents a compelling argument for designing the SKA such that it would offer imaging capabilities similar to those of other future telescopes. Imaging capabilities of the SKA are compared here with those of the major future as
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The Large Millimeter Telescope with outfitting running through 2006. The LMT will have nearly 2000m. of collecting area with an overall surface accuracy of 70 μm rms. Its sensitivity will exceed that of existing millimeter–wavelength telescopes by a significant margin. As a completely filled aperture, the LMT will have optimum s
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An Overview of the Submillimeter Array Telescopeea, Hawaii, near the CSO and JCMT facilities and was commissioned in November 2003 [2]. The array consists of eight 6-meter diameter antennas which can be moved among 24 pads on the sides of four Reuleaux triangles, producing a maximum angular resolution of 0″.1. Each antenna is equipped with a cryo
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Tunable Heterodyne Receivers - A Promising Outlook for Future Mid-Infrared Interferometry illustrated in Fig. 1 [1,2]. A local oscillator (LO) is precisely locked to a frequency close to the observing wavelength by the resonance of a Fabry-Perot diplexer, which itself is stabilised to a resonance of a special HeNe laser. The LO radiation with its known frequency is then superimposed ont
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ESPRIT – Exploratory Submillimeter sPace Radio Interferometric Telescope in the FIR, provides important and unique information on the star and planet formation process occurring in interstellar clouds, and the lifecycle of gas and dust in general. As these regions are heavily obscured by dust, FIR observations are the only means of getting insight in the physical condit
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