Very Long Baseline Interferometry with the SKA

Very Long Baseline Interferometry with the SKA
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DOI：
10.22323/1.215.0143
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发表时间：
2014-12
期刊：
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影响因子：
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通讯作者：
Z. Paragi;L. Godfrey;C. Reynolds;M. Rioja;A. Deller;Bo Zhang;L. Gurvits;M. Bietenholz;A. Szomoru;H. Bignall;P. Boven;P. Charlot;R. Dodson;S. Frey;M. Garrett;H. Imai;A. Lobanov;M. Reid;E. Ros;H. V. Langevelde;J. Zensus;Xing Zheng;A. Alberdi;I. Agudo;T. An;M. Argo;R. Beswick;A. Biggs;A. Brunthaler;R. M. Campbell;G. Cimò;F. Colomer;S. Corbel;J. Conway;D. Cseh;R. Deane;H. Falcke;K. Gabányi;M. Gawroński;M. Gaylard;G. Giovannini;M. Giroletti;C. Goddi;S. Goedhart;J. L. Gómez;A. Gunn;T. Jung;P. Kharb;H. Klockner;E. Kording;Y. Kovalev;M. Kunert‐Bajraszewska;M. Lindqvist;M. Lister;F. Mantovani;I. Martí-Vidal;M. Mezcua;J. McKean;E. Middelberg;J. Miller-Jones;J. Moldón;T. Muxlow;T. O’brien;M. P'erez-Torres;S. Pogrebenko;J. Quick;A. Rushton;R. Schilizzi;O. Smirnov;B. Sohn;G. Surcis;G. Taylor;S. Tingay;V. Tudose;A. Horst;J. V. Leeuwen;T. Venturi;R. Vermeulen;W. Vlemmings;A. D. Witt;O. Wucknitz;Jun Yang
Z. Paragi;L. Godfrey;C. Reynolds;M. Rioja;A. Deller;Bo Zhang;L. Gurvits;M. Bietenholz;A. Szomoru;H. Bignall;P. Boven;P. Charlot;R. Dodson;S. Frey;M. Garrett;H. Imai;A. Lobanov;M. Reid;E. Ros;H. V. Langevelde;J. Zensus;Xing Zheng;A. Alberdi;I. Agudo;T. An;M. Argo;R. Beswick;A. Biggs;A. Brunthaler;R. M. Campbell;G. Cimò;F. Colomer;S. Corbel;J. Conway;D. Cseh;R. Deane;H. Falcke;K. Gabányi;M. Gawroński;M. Gaylard;G. Giovannini;M. Giroletti;C. Goddi;S. Goedhart;J. L. Gómez;A. Gunn;T. Jung;P. Kharb;H. Klockner;E. Kording;Y. Kovalev;M. Kunert‐Bajraszewska;M. Lindqvist;M. Lister;F. Mantovani;I. Martí-Vidal;M. Mezcua;J. McKean;E. Middelberg;J. Miller-Jones;J. Moldón;T. Muxlow;T. O’brien;M. P'erez-Torres;S. Pogrebenko;J. Quick;A. Rushton;R. Schilizzi;O. Smirnov;B. Sohn;G. Surcis;G. Taylor;S. Tingay;V. Tudose;A. Horst;J. V. Leeuwen;T. Venturi;R. Vermeulen;W. Vlemmings;A. D. Witt;O. Wucknitz;Jun Yang
中科院分区：
其他
文献类型：
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作者：
Z. Paragi;L. Godfrey;C. Reynolds;M. Rioja;A. Deller;Bo Zhang;L. Gurvits;M. Bietenholz;A. Szomoru;H. Bignall;P. Boven;P. Charlot;R. Dodson;S. Frey;M. Garrett;H. Imai;A. Lobanov;M. Reid;E. Ros;H. V. Langevelde;J. Zensus;Xing Zheng;A. Alberdi;I. Agudo;T. An;M. Argo;R. Beswick;A. Biggs;A. Brunthaler;R. M. Campbell;G. Cimò;F. Colomer;S. Corbel;J. Conway;D. Cseh;R. Deane;H. Falcke;K. Gabányi;M. Gawroński;M. Gaylard;G. Giovannini;M. Giroletti;C. Goddi;S. Goedhart;J. L. Gómez;A. Gunn;T. Jung;P. Kharb;H. Klockner;E. Kording;Y. Kovalev;M. Kunert‐Bajraszewska;M. Lindqvist;M. Lister;F. Mantovani;I. Martí-Vidal;M. Mezcua;J. McKean;E. Middelberg;J. Miller-Jones;J. Moldón;T. Muxlow;T. O’brien;M. P'erez-Torres;S. Pogrebenko;J. Quick;A. Rushton;R. Schilizzi;O. Smirnov;B. Sohn;G. Surcis;G. Taylor;S. Tingay;V. Tudose;A. Horst;J. V. Leeuwen;T. Venturi;R. Vermeulen;W. Vlemmings;A. D. Witt;O. Wucknitz;Jun Yang

文献摘要

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将VLBI能力添加到SKA阵列将极大地拓宽SKA的科学领域，并且在当前规格范围内是可行的。SKA-VLBI最初可以通过为SKA1-MID和SKA1-SUR提供相控阵输出，并与其他射电望远镜一起使用这些极其敏感的站来实施，在SKA2中，可以通过实现分布式配置来提供长达数千公里的基线，并将其与现有的VLBI网络合并。本文描述了SKA-VLBI的动机和可能的实现。
Adding VLBI capability to the SKA arrays will greatly broaden the science of the SKA, and is feasible within the current specifications. SKA-VLBI can be initially implemented by providing phased-array outputs for SKA1-MID and SKA1-SUR and using these extremely sensitive stations with other radio telescopes, and in SKA2 by realising a distributed configuration providing baselines up to thousands of km, merging it with existing VLBI networks. The motivation for and the possible realization of SKA-VLBI is described in this paper.