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A LOFAR mini-survey for low-frequency radio emission from the nearest brown dwarfs

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posted on 2016-10-27, 10:32 authored by Ben Burningham, M. Hardcastle, J. D. Nichols, Sarah L. Casewell, S. P. Littlefair, C. Stark, M. R. Burleigh, S. Metchev, M. E. Tannock, R. J. V. Weeren, W. L. Williams, G. A. Wynn
We have conducted a mini-survey for low-frequency radio emission from some of the closest brown dwarfs to the Sun with rapid rotation rates: SIMP J013656.5+093347, WISEPC J150649.97+702736.0, and WISEPA J174124.26+255319.5. We have placed robust 3-sigma upper limits on the flux density in the 111 - 169 MHz frequency range for these targets: WISE 1506: < 0.72 mJy; WISE 1741: < 0.87 mJy; SIMP 0136: < 0.66 mJy. At 8 hours of integration per target to achieve these limits, we find that systematic and detailed study of this class of object at LOFAR frequencies will require a substantial dedication of resources.

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Citation

Monthly Notices of the Royal Astronomical Society, 2016, 463 (2), pp. 2202-2209

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Monthly Notices of the Royal Astronomical Society

Publisher

Oxford University Press (OUP)

issn

0035-8711

eissn

1365-2966

Acceptance date

2016-08-12

Copyright date

2016

Available date

2016-10-27

Publisher version

http://mnras.oxfordjournals.org/content/463/2/2202

Language

en

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