Sky model of Cygnus A extracted from LOFAR-HBA observations at 110–250 MHz
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This Cygnus A model is a high-resolution (5 arcsec), spectrally varying sky model derived from LOFAR HBA observations in the 110–250 MHz range. It was built using the WSClean multi-scale and multi-frequency deconvolution with forced-spectrum fitting (Ceccotti et al. 2023), incorporating spatially varying spectral indices and curvature. The total flux has been scaled to match McKean et al (2016) in the 10–300 MHz range.
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Zenodo创建时间：
2025-02-17
