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008 150903s2012 gw | o |||| 0|eng d
020 _a9783642227950
_99783642227950
024 7 _a10.1007/9783642227950
_2doi
035 _avtls000357537
039 9 _a201509030558
_bVLOAD
_c201405070217
_dVLOAD
_y201402191318
_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB4
100 1 _aBarbosa, Domingos.
_eeditor.
_9343460
245 1 4 _aThe Square Kilometre Array: Paving the way for the new 21st century radio astronomy paradigm :
_bProceedings of Symposium 7 of JENAM 2010 /
_cedited by Domingos Barbosa, Sonia Anton, Leonid Gurvits, Dalmiro Maia.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c2012.
300 _ax, 116 páginas 31 ilustraciones
_brecurso en línea.
336 _atexto
_btxt
_2rdacontent
337 _acomputadora
_bc
_2rdamedia
338 _arecurso en línea
_bcr
_2rdacarrier
347 _aarchivo de texto
_bPDF
_2rda
490 0 _aAstrophysics and Space Science Proceedings,
_x1570-6591
500 _aSpringer eBooks
505 0 _aThe SKA Challenge -- The SKA new Instrumentation; Aperture Arrays -- AGN, Star Formation, and the nanoJy Sky -- Using HI absorption to trace outflows from galaxies and feeding of AGN -- Galaxy Dynamics -- Transient Phenomena: Opportunities for New Discoveries -- Cosmic Magnetism: Current Status and Outlook to the SKA -- The SKA and “High-Resolution” Science -- Precision Astrometry: from VLBI to Gaia and SKA -- Ultra Steep Spectrum radio sources in the Lockman Hole: SERVS identifications and redshift distribution at the faintest radio fluxes -- Probing the Very First Galaxies with the SKA.
520 _aThe Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telescope over a wavelength range of several hundred to one, from decametric to microwave wavelengths. It will revolutionize the study of the most abundant element in the Universe, hydrogen, from the epoch of reionisation to the present-day, probing the onset formation period of the very first stars, will closely scan proto-planets and, through the precision timing of pulsars, will detect the distortions of space-time due to gravitational radiation. The SKA is a sensing network spanning 3000 km from its centre and with a collecting area of more than 1 square kilometre, using technologies of the 21st century. The SKA will make the study of a wide range of phenomena initially studied at other wavelengths possible at radio wavelengths, as well as opening a new discovery window on new phenomena at radio wavelengths. Symposium 7 of the JENAM 2010 aimed at bringing these diverse opportunities to the attention of both theoretical and observational astronomers working at all wavelengths, including the potential for synergies with other facilities. The meeting ·        highlighted the scientific potential of the SKA ·        discussed  scientific priorities and their impact on the design of the SKA ·        explored the synergies between the SKA and other next-generation astronomical facilities in different wavelength domains such as the ALMA, ELTs, LSST, JWST, GRE, IXO, Gaia and Euclid, and high-energy facilities (Auger) ·        explored the “cyber–infrastructure” that may become available for the distribution and distributed analysis of SKA data
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700 1 _aAnton, Sonia.
_eeditor.
_9343461
700 1 _aGurvits, Leonid.
_eeditor.
_9343462
700 1 _aMaia, Dalmiro.
_eeditor.
_9343463
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9783642227943
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-3-642-22795-0
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999 _c304584
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