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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004540naa a2200493 4500
001oai:research.chalmers.se:882ee71f-15f2-487b-adbe-dcd108777977
003SwePub
008171007s2014 | |||||||||||000 ||eng|
024a https://research.chalmers.se/publication/2422992 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a kon2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Hoare, M. G.u University of Leeds4 aut
2451 0a The cradle of life and the SKA
264 1c 2014
520 a We provide an overview of the exciting capabilities of the SKA in the Cradle of Life theme. With the deployment of the high frequency band 5 receivers, the phase 1 of the SKA can conduct headline science in the study of the earliest stages of grain growth in proto-planetary disks. SKA1-MID can map the 2 cm continuum emission at a resolution of 4 au in the nearest systems and therefore begin to probe the distribuion of cm-sized particles across the snow line. This frequency range will also enable deep searches for pre-biotic molecules such as amino acids from pre-stellar cores to the cold, outer regions of proto-planetary disks where cometary material forms. The lowest frequency capabilities of SKA1 can be used to examine the magnetic fields of exo-planets via their auroral radio emission. This gives unique insight into their interiors and could potentially detect exo-moons. Across the full frequency range, the SKA1 will also carry out systematic, volume-limited searches of exo-planet systems for signals from technologically advanced civilizations. The sensitivity of SKA1 means that these only need to be at the level of typical airport radar signals in the nearest systems. Hence, the SKA1 can conduct high impact science from the first steps on the road to planets and life, through areas affecting the habitability of planets, and ultimately, to whether we are alone in the Galaxy. These inspirational themes will greatly help in the effort to bring SKA1 science to a wide audience and to ensure the progression to the full SKA.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
700a Perez, L.u National Radio Astronomy Observatory4 aut
700a Bourke, T. L.4 aut
700a Testi, L.u Ludwig-Maximilians-Universität München,Ludwig Maximilian University of Munich,European Southern Observatory (ESO),Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory4 aut
700a Jimenez-Serra, I.u University College London (UCL),European Southern Observatory (ESO)4 aut
700a Zarka, P.u LESIA - Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique4 aut
700a Siemion, A.u Radboud Universiteit,Radboud University,University of California,Netherlands Institute for Radio Astronomy (ASTRON)4 aut
700a Langevelde, H. J. V.u JIVE,Universiteit Leiden (UL),Leiden University (UL)4 aut
700a Loinard, L.u Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico4 aut
700a Anglada, G.u Instituto de Astrofisica de Andalucía (IAA),Institute of Astrophysics of Andalusia (IAA)4 aut
700a Belloche, A.4 aut
700a Bergman, Per,d 1960u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)pbergman
700a Booth, Roy,d 1938u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)roy
700a Caselli, P.4 aut
700a Chandler, C. J.u National Radio Astronomy Observatory4 aut
700a Codella, C.u Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory4 aut
700a Hallinan, G.u California Institute of Technology (Caltech)4 aut
700a Lazio, J.u California Institute of Technology (Caltech)4 aut
700a Morrison, I. S.u University of New South Wales (UNSW),Swinburne University of Technology4 aut
700a Podio, L.u Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory4 aut
700a Remijan, A.u National Radio Astronomy Observatory4 aut
700a Tarter, J.u SETI Institute4 aut
710a University of Leedsb National Radio Astronomy Observatory4 org
773t Proceedings of Scienceg 9-13-June-2014q 9-13-June-2014x 1824-8039
8564 8u https://research.chalmers.se/publication/242299

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