Download | - View final version: The ASKAP-EMU Early Science Project: 888 MHz radio continuum survey of the Large Magellanic Cloud (PDF, 5.3 MiB)
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DOI | Resolve DOI: https://doi.org/10.1093/mnras/stab1858 |
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Author | Search for: Pennock, Clara MORCID identifier: https://orcid.org/0000-0003-2164-5337; Search for: van Loon, Jacco Th; Search for: Filipović, Miroslav D; Search for: Andernach, HeinzORCID identifier: https://orcid.org/0000-0003-4873-1681; Search for: Haberl, Frank; Search for: Kothes, Roland1; Search for: Lenc, EmilORCID identifier: https://orcid.org/0000-0002-9994-1593; Search for: Rudnick, LawrenceORCID identifier: https://orcid.org/0000-0001-5636-7213; Search for: White, Sarah VORCID identifier: https://orcid.org/0000-0002-2340-8303; Search for: Agliozzo, ClaudiaORCID identifier: https://orcid.org/0000-0003-1749-2542; Search for: Antón, Sonia; Search for: Bojičić, Ivan; Search for: Bomans, Dominik J; Search for: Collier, Jordan DORCID identifier: https://orcid.org/0000-0002-2326-7432; Search for: Crawford, Evan JORCID identifier: https://orcid.org/0000-0001-5197-1091; Search for: Hopkins, Andrew M; Search for: Jeganathan, Kanapathippillai; Search for: Kavanagh, Patrick J; Search for: Koribalski, Bärbel SORCID identifier: https://orcid.org/0000-0003-4351-993X; Search for: Leahy, DenisORCID identifier: https://orcid.org/0000-0002-4814-958X; Search for: Maggi, Pierre; Search for: Maitra, ChandreyeeORCID identifier: https://orcid.org/0000-0002-0766-7313; Search for: Marvil, Josh; Search for: Michałowski, Michał JORCID identifier: https://orcid.org/0000-0001-9033-4140; Search for: Norris, Ray P; Search for: Oliveira, Joana MORCID identifier: https://orcid.org/0000-0002-0861-7094; Search for: Payne, Jeffrey L; Search for: Sano, Hidetoshi; Search for: Sasaki, ManamiORCID identifier: https://orcid.org/0000-0001-5302-1866; Search for: Staveley-Smith, ListerORCID identifier: https://orcid.org/0000-0002-8057-0294; Search for: Vardoulaki, EleniORCID identifier: https://orcid.org/0000-0002-4437-1773 |
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Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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Funder | Search for: STFC; Search for: National Science Foundation; Search for: University of Minnesota; Search for: COMPETE; Search for: Jet Propulsion Laboratory; Search for: California Institute of Technology; Search for: National Aeronautics and Space Administration |
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Format | Text, Article |
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Subject | surveys; planetary nebulae: general; Magellanic Clouds; radio continuum: galaxies; radio continuum: ISM; radio continuum: stars |
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Abstract | We present an analysis of a new 120 deg² radio continuum image of the Large Magellanic Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of 13′′.9 × 12′′.1 from the Australian Square Kilometre Array Pathfinder processed as part of the Evolutionary Map of the Universe survey. The median root mean squared noise is 58 μJy beam⁻¹. We present a catalogue of 54 612 sources, divided over a Gold list (30 866 sources) complete down to 0.5 mJy uniformly across the field, a Silver list (22 080 sources) reaching down to <0.2 mJy, and a Bronze list (1666 sources) of visually inspected sources in areas of high noise and/or near bright complex emission. We discuss detections of planetary nebulae and their radio luminosity function, young stellar objects showing a correlation between radio luminosity and gas temperature, novae and X-ray binaries in the LMC, and active stars in the Galactic foreground that may become a significant population below this flux level. We present examples of diffuse emission in the LMC (H II regions, supernova remnants, bubbles) and distant galaxies showcasing spectacular interaction between jets and intracluster medium. Among 14 333 infrared counterparts of the predominantly background radio source population, we find that star-forming galaxies become more prominent below 3 mJy compared to active galactic nuclei. We combine the new 888 MHz data with archival Australia Telescope Compact Array data at 1.4 GHz to determine spectral indices; the vast majority display synchrotron emission but flatter spectra occur too. We argue that the most extreme spectral index values are due to variability. |
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Publication date | 2021-07-02 |
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Publisher | Royal Astronomical Society Oxford University Press |
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Licence | |
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In | |
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Language | English |
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Peer reviewed | Yes |
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Export citation | Export as RIS |
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Report a correction | Report a correction (opens in a new tab) |
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Record identifier | 79b840f2-6629-4db1-ad65-ecba9635f600 |
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Record created | 2022-11-04 |
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Record modified | 2022-11-04 |
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