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Impact of Residual Gain Errors on the Detectability of Ionized Bubbles during Reionization with SKA 21-cm observations
Detecting ionized bubbles and characterizing their properties and the surrounding intergalactic medium (IGM) using the HI 21-cm signal provides direct probes of cosmic reionization. Here, we focus on the detection of individual ionized bubbles around luminous sources using a matched-filter technique
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