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

Ben Burningham; M. Hardcastle; J. D. Nichols; S. L. Casewell; S. P. Littlefair; Craig R. Stark; M. R. Burleigh; S. Metchev; M. E. Tannock; R. J. van Weeren; W. L. Williams; G. A. Wynn

doi:10.1093/mnras/stw2065

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

Ben Burningham, M. Hardcastle, J. D. Nichols, S. L. Casewell, S. P. Littlefair, Craig R. Stark, M. R. Burleigh, S. Metchev, M. E. Tannock, R. J. van Weeren, W. L. Williams, G. A. Wynn

SDI - Games and Arts

Research output: Contribution to journal › Article › peer-review

6 Citations (Scopus)

53 Downloads (Pure)

Abstract

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 150649.97+702736.0, and WISEPA J174124.26+255319.5.We have placed robust 3s 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.

Original language	English
Pages (from-to)	2202–2209
Number of pages	8
Journal	Monthly Notices of the Royal Astronomical Society
Volume	463
Issue number	2
Early online date	19 Aug 2016
DOIs	https://doi.org/10.1093/mnras/stw2065
Publication status	Published - 1 Dec 2016

Access to Document

10.1093/mnras/stw2065Licence: CC BY

Stark_aLOFARminisurvey_Published_2016Final published version, 1.09 MBLicence: CC BY

Craig Stark
- C516967@abertay.ac.uk
- SDI - Games Technology & Mathematics - Lecturer
Person: Academic

Cite this

Burningham, B., Hardcastle, M., Nichols, J. D., Casewell, S. L., Littlefair, S. P., Stark, C. R., Burleigh, M. R., Metchev, S., Tannock, M. E., van Weeren, R. J., Williams, W. L., & Wynn, G. A. (2016). A LOFAR mini-survey for low-frequency radio emission from the nearest brown dwarfs. Monthly Notices of the Royal Astronomical Society, 463(2), 2202–2209. https://doi.org/10.1093/mnras/stw2065

Burningham, Ben ; Hardcastle, M. ; Nichols, J. D. ; Casewell, S. L. ; Littlefair, S. P. ; Stark, Craig R. ; Burleigh, M. R. ; Metchev, S. ; Tannock, M. E. ; van Weeren, R. J. ; Williams, W. L. ; Wynn, G. A. / A LOFAR mini-survey for low-frequency radio emission from the nearest brown dwarfs. In: Monthly Notices of the Royal Astronomical Society. 2016 ; Vol. 463, No. 2. pp. 2202–2209.

@article{8d966761655b43d1998c4b6355edb218,

title = "A LOFAR mini-survey for low-frequency radio emission from the nearest brown dwarfs",

abstract = "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 150649.97+702736.0, and WISEPA J174124.26+255319.5.We have placed robust 3s 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.",

author = "Ben Burningham and M. Hardcastle and Nichols, {J. D.} and Casewell, {S. L.} and Littlefair, {S. P.} and Stark, {Craig R.} and Burleigh, {M. R.} and S. Metchev and Tannock, {M. E.} and {van Weeren}, {R. J.} and Williams, {W. L.} and Wynn, {G. A.}",

year = "2016",

month = dec,

day = "1",

doi = "10.1093/mnras/stw2065",

language = "English",

volume = "463",

pages = "2202–2209",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "2",

}

Burningham, B, Hardcastle, M, Nichols, JD, Casewell, SL, Littlefair, SP, Stark, CR, Burleigh, MR, Metchev, S, Tannock, ME, van Weeren, RJ, Williams, WL & Wynn, GA 2016, 'A LOFAR mini-survey for low-frequency radio emission from the nearest brown dwarfs', Monthly Notices of the Royal Astronomical Society, vol. 463, no. 2, pp. 2202–2209. https://doi.org/10.1093/mnras/stw2065

A LOFAR mini-survey for low-frequency radio emission from the nearest brown dwarfs. / Burningham, Ben; Hardcastle, M.; Nichols, J. D.; Casewell, S. L.; Littlefair, S. P.; Stark, Craig R.; Burleigh, M. R.; Metchev, S.; Tannock, M. E.; van Weeren, R. J.; Williams, W. L.; Wynn, G. A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 463, No. 2, 01.12.2016, p. 2202–2209.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

T1 - A LOFAR mini-survey for low-frequency radio emission from the nearest brown dwarfs

AU - Burningham, Ben

AU - Hardcastle, M.

AU - Nichols, J. D.

AU - Casewell, S. L.

AU - Littlefair, S. P.

AU - Stark, Craig R.

AU - Burleigh, M. R.

AU - Metchev, S.

AU - Tannock, M. E.

AU - van Weeren, R. J.

AU - Williams, W. L.

AU - Wynn, G. A.

PY - 2016/12/1

Y1 - 2016/12/1

N2 - 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 150649.97+702736.0, and WISEPA J174124.26+255319.5.We have placed robust 3s 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.

AB - 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 150649.97+702736.0, and WISEPA J174124.26+255319.5.We have placed robust 3s 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.

U2 - 10.1093/mnras/stw2065

DO - 10.1093/mnras/stw2065

M3 - Article

VL - 463

SP - 2202

EP - 2209

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -

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

Abstract

Access to Document

Fingerprint

Profiles

Craig Stark

Cite this