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Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1)

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arxiv 1912.12699 v1 pith:TWTNRMX3 submitted 2019-12-29 astro-ph.IM

Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1)

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keywords anticipatedarraydesigninformationkilometreperformancephaseska1
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The Square Kilometre Array (SKA), currently under design, will be a transformational facility for studying the Universe at centimetre and metre wavelengths in the next decade and beyond. This paper provides the current best estimate of the anticipated performance of SKA Phase 1 (SKA1), using detailed design work, before actual on-sky measurements have been made. It will be updated as new information becomes available. The information contained in this paper takes precedent over any previous documents.

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Cited by 52 Pith papers

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  15. Radio Emission from High-Frequency Gravitational Wave Point Sources

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  18. The CatWISE2020 Quasar dipole: A Reassessment of the Cosmic Dipole Anomaly

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  35. Probing Neutron Star Interiors and the Properties of Cold Ultra-dense Matter with the SKAO

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  36. Advancing extragalactic spectral line studies with the Square Kilometre Array Observatory

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    SKAO will extend maser, molecular, recombination-line and isotope studies across cosmic time, with AA4 and a high-frequency extension enabling transformative surveys including possible HeH+ detection.

  37. Enhancing VLBI Capability with the SKA-Mid and the Jingdong 120-m Radio Telescope

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  41. Discovering and Characterising Exoplanets and Ultracool Dwarfs with the Square Kilometre Array

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    The Square Kilometre Array is projected to enable first radio detections of giant exoplanets, thousands of ultracool dwarfs, and few-Earth-mass planets around nearby UCDs via VLBI astrometry.

  42. Measurements of magnetic fields in circumnuclear matter with the SKA telescopes

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    SKA-Mid/Low plus VLBI should enable Zeeman and broadband RM measurements of AGN circumnuclear magnetic fields from ~100 pc disks down to sub-pc scales that current instruments largely cannot reach.

  43. Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era

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  44. Radio Wave Propagation as a Probe of the Solar Corona and Solar Wind

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  45. Fast Radio Bursts as Cosmological Probes

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  46. Probing Anomalous Microwave Emission with the Square Kilometre Array

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    This review summarizes evidence for anomalous microwave emission and projects how SKA observations will identify its carriers and mechanisms in Galactic and extragalactic environments.

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    astro-ph.GA 2026-06 unverdicted novelty 2.0

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  49. Probing Physical Conditions in Classical and Symbiotic Novae with the Square Kilometre Array Observatory

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    SKAO will enable regular multi-frequency radio monitoring of Galactic novae to probe ionised and relativistic particle populations in classical and symbiotic systems.

  50. Solar Radio Burst Fine Structures

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    Recent sub-second imaging spectroscopy of solar radio burst fine structures challenges existing theoretical models, with the SKA positioned to enable new frameworks for electron acceleration and coronal turbulence.

  51. Probing Merger Shocks in Galaxy Clusters in the SKA Era

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  52. Opening new parameter space windows on galaxy/AGN co-evolution with SKA radio continuum surveys

    astro-ph.GA 2026-06 unverdicted novelty 1.0

    Overview of SKAO radio surveys for galaxy/AGN co-evolution, including tiered surveys, multi-frequency imaging, and synergies with other observatories.