Scientific research

MeerKAT Radio Observations of ESO 137-006

MeerKAT radio telescope visibility data for the radio galaxy ESO 137-006, located in the Norma galaxy cluster (Abell 3627) at a distance of approximately 70 megaparsecs. The observations cover two frequency bands (980–1080 MHz and 1356–1440 MHz) and comprise 14 hours of on-target integration time taken in May 2019 using all 64 MeerKAT antennas. These data led to the discovery of multiple collimated synchrotron threads (CSTs) — narrow, thread-like structures of radio emission connecting the galaxy's radio lobes — a configuration not previously observed in radio galaxies (Ramatsoku et al. 2020, A&A 636, L1). The data are stored in...

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Data coverage

MeerKAT radio telescope visibility data for the radio galaxy ESO 137-006, located in the Norma galaxy cluster (Abell 3627) at a distance of approximately 70 megaparsecs. The observations cover two frequency bands (980–1080 MHz and 1356–1440 MHz) and comprise 14 hours of on-target integration time taken in May 2019 using all 64 MeerKAT antennas. These data led to the discovery of multiple collimated synchrotron threads (CSTs) — narrow, thread-like structures of radio emission connecting the galaxy's radio lobes — a configuration not previously observed in radio galaxies (Ramatsoku et al. 2020, A&A 636, L1). The data are stored in Zarr format, implementing the CASA Measurement Set v2 data model. They are cloud-native and can be accessed directly from S3 using the dask-ms Python library without prior download. The dataset consists of three Measurement Sets: one primary calibrator and two target-field observations. Each target dataset is about 1.1TB compressed (~3TB uncompressed). A key community challenge associated with this dataset is performing distributed radio interferometric imaging (gridding, FFT, deconvolution) at scale directly on cloud storage — a workflow directly relevant to future Square Kilometre Array (SKA) pipelines.

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Creative Commons Attribution 4.0 International (CC BY 4.0). Attribution required for refereed scientific publications — please cite Ramatsoku et al. (2020), A&A 636, L1, https://doi.org/10.1051/0004-6361/202037800.

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