proceeding

Euclid & SKA Synergies

T. KitchingUniversity College London, Department of Space and Climate Physics;David BaconICG , University of Portsmouth ;Michael L. BrownDepartment of Physics , University of Manchester ;Philip BullUniversity of Oslo , Institute for Theoretical Astrophysics ;Jason D. McEwenUniversity College London , Department of Space and Climate Physics ;Masmune OguriGraduate School of Science, University of Tokyo, Japan;R. ScaramellaINAF-Osservatorio di Roma, I-00040 Monteporzio Catone, Italy;Keitaro TakahashiGraduate School of Science and Technology, Kumamoto University, Japan;Kinwah WuUniversity College London, Department of Space and Climate Physics;Daisuke YamauchiResearch Center for the Early Universe, University of Tokyo, Japan;

2015en

Ochiq kirishGibrid

Litsenziya: cc-by-nc-sa

ABI

Annotatsiya

Over the past few years two of the largest and highest fidelity experiments conceived have been approved for construction: Euclid is an ESA M-Class mission that will map three-quarters of the extra galactic sky with Hubble Space Telescope resolution optical and NIR imaging, and NIR spectroscopy, its scientific aims (amongst others) are to create a map of the dark Universe and to determine the nature of dark energy. The Square Kilometre Array (SKA) has similar scientific aims (and others) using radio wavelength observations. The two experiments are synergistic in several respects, both through the scientific objectives and through the control of systematic effects. SKA Phase-1 and Euclid will be commissioned on similar timescales offering an exciting opportunity to exploit synergies between these facilities.

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Identifikatorlar

DOI: 10.22323/1.215.0146

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