Next-generation continuum surveys will be strongly constrained by dynamic range and confusion. For example, the ASKAP-EMU (Evolutionary Map of the Universe) project will map 75% of the sky at 20cm to a sensitivity of 10 microJy - some 45 times deeper than NVSS, and is likely to be challenged by issues of confusion, cross-identification, and dynamic range. Here we describe the survey, the issues, and the steps that can be taken to overcome them. We also explore ways of using multiwavelength data to penetrate well beyond the classical confusion limit, using multiwavelength data, and an innovative outreach approach to cross-identification.
Theoretical Estimates of Integrated Sachs-Wolfe Effect Detection through EMU-ASKAP Survey with Confusion, Position Uncertainty, Shot Noise and SNR analysis
Number counts, confusion, mapping issues and sky coverage analysis for radio continuum surveys through EMU Early Science, EMU-ASKAP, and WODAN especially for cosmology science goals
The Abell 3391/95 galaxy cluster system: A 15 Mpc intergalactic medium emission filament, a warm gas bridge, infalling matter clumps, and (re-) accelerated plasma discovered by combining SRG/eROSITA data with ASKAP/EMU and DECam data
Accelerated expansion of the universe and chasing photons from the CMB to study the late time integrated Sachs-Wolfe effect over different redshift ranges
RG-CAT: Detection Pipeline and Catalogue of Radio Galaxies in the EMU Pilot Survey
Western Sydney University（西悉尼大学）；CSIRO Data61（澳大利亚联邦科学与工业研究组织Data61部）；International Centre for Radio Astronomy Research（国际射电天文学研究中心）；The University of Western Australia（西澳大学）；Macquarie University（麦考瑞大学）；Universidad de Guanajuato（瓜纳华托大学）；University of Wisconsin-Madison（威斯康星大学麦迪逊分校）；INAF-Osservatorio Astrofisico di Catania（意大利国家天体物理研究所卡塔尼亚天体观测台）；National Radio Astronomy Observatory（国家射电天文台）；University of Tasmania（塔斯马尼亚大学）
