Exploring the cosmic frontier : astrophysical instruments for the 21st century
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 optic...
Uloženo v:
| Hlavní autoři: | , |
|---|---|
| Médium: | Livre numérique |
| Jazyk: | Anglais |
| Vydáno: |
Berlin, Heidelberg :
Springer Berlin Heidelberg
[20..].
Cham : Springer Nature |
| Vydání: | 1st ed. 2007. |
| Edice: | ESO Astrophysics Symposia European Southern Observatory
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| On-line přístup: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Poznámka: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Exploring the cosmic frontier, astrophysical instruments for the 21st century, A.P. Lobanov, J.A. Zensus, C. Cesarsky... [et al.] (Eds.), Berlin, Springer, 2007, 1 vol.(XXVIII-270 p.), ESO astrophysics symposia, 978-3-540-39755-7 |
Obsah:
- Future Astrophysical Facilities Radio Astronomy Facilities Future Optical and Near-Infrared Facilities The New 40-m Radiotelescope of OAN in Yebes, Spain Design of the Near-term Next Generation Space-VLBI Mission VSOP-2 Imaging Across the Spectrum: Synergies Between SKA and Other Future Telescopes The Korean VLBI Network Project Frequency Protection for the 21st Century SCUBA-2: A Large-Format CCD-Style Imager for Submillimeter Astronomy The Large Millimeter Telescope An Overview of the Submillimeter Array Telescope Tunable Heterodyne Receivers - A Promising Outlook for Future Mid-Infrared Interferometry ESPRIT Exploratory Submillimeter sPace Radio Interferometric Telescope Fizeau Interferometry with the LBT Astronomy on the Way to ELTs MUSE: 3D Spectroscopy with Large Telescopes Layer-Oriented MCAO Projects for 8-m Class Telescopes and Possible Scientific Outcome Prospects for an Extremely Large Synthesis Array Interferometry in the Near-Infrared: 1 Mas Resolution at the Wavelength of 1 Micron Electrical and Geometrical Characterization of the Silicon Flight Sensors of the GLAST/LAT Tracking System Environmental Testing of the GLAST Tracker Subsystem The Potential of a Large Cherenkov Array for Supersymmetry and Cosmology MAGIC: First Observational Results and Perspectives for Future Developments LOBSTER - Astrophysics with Lobster Eye Telescopes Novel Light-Weight X-ray Optics for Future X-ray Telescopes GLAST LAT Science Prospects Astrophysics with Astronomical Plate Archives Virtual Observatories and Access to Radio Interferometry Data Fundamental Physics and Cosmology Fundamental Physics with the SKA: Strong-Field Tests of Gravity Using Pulsars and Black Holes Measuring Variations in the Fundamental Constants with the Square Kilometre Array ELT Observations of Supernovae at the Edge of the Universe SKA and the Magnetic Universe SSF as a Manifestation of Protoobjects in the Dark Ages Epoch: Theory and Experiment Cosmic Ray Astrophysics with AMS-02 Studying the Nature of Dark Energy with Current and Future Instruments Project ASTRAL: All-sky Space Telescope to Record Afterglow Locations High-redshift Universe, Galaxies, Galaxy Evolution Overview of the Science Case for a 50 100m Extremely Large Telescope Distant Galaxies and Extremely Large Telescopes Extragalactic Science with the Allen Telescope Array Spectral Aging in the Relic Radio Galaxy B2 0924+30 Extragalactic Sources with Extended Radio Emission The B3VLA Sample at Low Frequencies: Results from a Survey at 74 MHz Modeling the Faint Radio Population: The NanoJY Radio Sky Radio View of Merging Clusters of Galaxies AGN and Compact Objects Active Galactic Nuclei at the Crossroads of Astrophysics New Frontiers in AGN Astrophysics: The X-ray Perspective Deep Radio Source Surveys with the SKA e-VLBI a Wide-Field Imaging Instrument with Milliarcsecond Resolution & Microjy Sensitivity Results from Observations of AGNs with the H·E·S·S· Telescope System and Future Plans