ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.25917/cm5z-ds40&rft.title=MWA GLEAM Survey Raw Data 2013-2015&rft.identifier=10.25917/cm5z-ds40&rft.publisher=Curtin University&rft.description=The GaLactic and Extragalactic All-sky MWA (GLEAM) survey comprises three months of observations spread over three years using the MWA between 72 and 231 MHz. The surveyed area includes all sky south of declination 30deg and each part of the sky is revisted at least three times. About 50% of the data have been processed and published in continuum catalogues by Hurley-Walker et al. (2017, 2019c) and Franzen et al. (2021). This collection concerns the raw data which comprises these publications, and additional data which has not yet been processed. Retaining the raw data is important for scientific reproducibility. Additionally, it will be necessary to fill in the short baselines (corresponding to large angular scales) in the GLEAM-eXtended survey, currently funded by an ARC Future Fellowship until December 2024. The data are also useful for transient and variability searches and to understand how ionospheric conditions at the future SKA site vary as a function of solar activity.&rft.creator=Anonymous&rft.date=2022&rft_rights=&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft_subject=Galactic astronomy&rft_subject=Cosmology and extragalactic astronomy&rft.type=dataset&rft.language=English Access the data

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The GaLactic and Extragalactic All-sky MWA (GLEAM) survey comprises three months of observations spread over three years using the MWA between 72 and 231 MHz. The surveyed area includes all sky south of declination 30deg and each part of the sky is revisted at least three times. About 50% of the data have been processed and published in continuum catalogues by Hurley-Walker et al. (2017, 2019c) and Franzen et al. (2021). This collection concerns the raw data which comprises these publications, and additional data which has not yet been processed. Retaining the raw data is important for scientific reproducibility. Additionally, it will be necessary to fill in the short baselines (corresponding to large angular scales) in the GLEAM-eXtended survey, currently funded by an ARC Future Fellowship until December 2024. The data are also useful for transient and variability searches and to understand how ionospheric conditions at the future SKA site vary as a function of solar activity.

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