Abstract
SN 2023ixf is a Type II-L supernova that occurred in M101 in 2023 May. The European VLBI Network (EVN) observed SN 2023ixf at 5 GHz approximately one month later, on June 28. We calibrated the EVN data using AIPS and CASA, reporting non-detection of a radio source with 5σ flux upper limits of 113 μJy and 135 μJy for both pipelines, respectively.
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