Limits on low-frequency radio emission from southern exoplanets with the murchison widefield array
Murphy, T
Bell, ME
Kaplan, DL
Gaensler, BM
Offringa, AR
Lenc, E
Hurley-Walker, N
Bernardi, G
Bowman, JD
Briggs, F
Cappallo, RJ
Corey, BE
Deshpande, AA
Emrich, D
Goeke, R
Greenhill, LJ
Hazelton, BJ
Hewitt, JN
Johnston-Hollitt, M
Kasper, JC
Kratzenberg, E
Lonsdale, CJ
Lynch, MJ
McWhirter, SR
Mitchell, DA
Morales, MF
Morgan, E
Oberoi, D
Ord, SM
Prabu, T
Rogers, AEE
Roshi, DA
Udaya Shankar, N
Srivani, KS
Subrahmanyan, R
Tingay, SJ
Waterson, M
Wayth, RB
Webster, RL
Whitney, AR
Williams, A
Williams, CL
- Publication Type:
- Journal Article
- Citation:
- Monthly Notices of the Royal Astronomical Society, 2015, 446 (3), pp. 2560 - 2565
- Issue Date:
- 2015-01-01
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Full metadata record
Field | Value | Language |
---|---|---|
dc.contributor.author | Murphy, T | en_US |
dc.contributor.author |
Bell, ME |
en_US |
dc.contributor.author | Kaplan, DL | en_US |
dc.contributor.author | Gaensler, BM | en_US |
dc.contributor.author | Offringa, AR | en_US |
dc.contributor.author | Lenc, E | en_US |
dc.contributor.author | Hurley-Walker, N | en_US |
dc.contributor.author | Bernardi, G | en_US |
dc.contributor.author | Bowman, JD | en_US |
dc.contributor.author | Briggs, F | en_US |
dc.contributor.author | Cappallo, RJ | en_US |
dc.contributor.author | Corey, BE | en_US |
dc.contributor.author | Deshpande, AA | en_US |
dc.contributor.author | Emrich, D | en_US |
dc.contributor.author | Goeke, R | en_US |
dc.contributor.author | Greenhill, LJ | en_US |
dc.contributor.author | Hazelton, BJ | en_US |
dc.contributor.author | Hewitt, JN | en_US |
dc.contributor.author | Johnston-Hollitt, M | en_US |
dc.contributor.author | Kasper, JC | en_US |
dc.contributor.author | Kratzenberg, E | en_US |
dc.contributor.author | Lonsdale, CJ | en_US |
dc.contributor.author | Lynch, MJ | en_US |
dc.contributor.author | McWhirter, SR | en_US |
dc.contributor.author | Mitchell, DA | en_US |
dc.contributor.author | Morales, MF | en_US |
dc.contributor.author | Morgan, E | en_US |
dc.contributor.author | Oberoi, D | en_US |
dc.contributor.author | Ord, SM | en_US |
dc.contributor.author | Prabu, T | en_US |
dc.contributor.author | Rogers, AEE | en_US |
dc.contributor.author | Roshi, DA | en_US |
dc.contributor.author | Udaya Shankar, N | en_US |
dc.contributor.author | Srivani, KS | en_US |
dc.contributor.author | Subrahmanyan, R | en_US |
dc.contributor.author | Tingay, SJ | en_US |
dc.contributor.author | Waterson, M | en_US |
dc.contributor.author | Wayth, RB | en_US |
dc.contributor.author | Webster, RL | en_US |
dc.contributor.author | Whitney, AR | en_US |
dc.contributor.author | Williams, A | en_US |
dc.contributor.author | Williams, CL | en_US |
dc.date.issued | 2015-01-01 | en_US |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society, 2015, 446 (3), pp. 2560 - 2565 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/10453/132087 | |
dc.description.abstract | © 2014 The Authors. We present the results of a survey for low-frequency radio emission from 17 known exoplanetary systems with the Murchison Widefield Array. This sample includes 13 systems that have not previously been targeted with radio observations. We detected no radio emission at 154 MHz, and put 3τ upper limits in the range 15.2-112.5 mJy on this emission. We also searched for circularly polarized emission and made no detections, obtaining 3τ upper limits in the range 3.4-49.9 mJy. These are comparable with the best low-frequency radio limits in the existing literature and translate to luminosity limits of between 1.2 × 1014 and 1.4 × 1017 Wif the emission is assumed to be 100 per cent circularly polarized. These are the first results from a larger program to systematically search for exoplanetary emission with the MWA. | en_US |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | en_US |
dc.relation.isbasedon | 10.1093/mnras/stu2253 | en_US |
dc.subject.classification | Astronomy & Astrophysics | en_US |
dc.title | Limits on low-frequency radio emission from southern exoplanets with the murchison widefield array | en_US |
dc.type | Journal Article | |
utslib.citation.volume | 3 | en_US |
utslib.citation.volume | 446 | en_US |
utslib.for | 0201 Astronomical and Space Sciences | en_US |
pubs.embargo.period | Not known | en_US |
pubs.organisational-group | /University of Technology Sydney | |
pubs.organisational-group | /University of Technology Sydney/Faculty of Science | |
pubs.organisational-group | /University of Technology Sydney/Faculty of Science/School of Mathematical and Physical Sciences | |
utslib.copyright.status | open_access | |
pubs.issue | 3 | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 446 | en_US |
Abstract:
© 2014 The Authors. We present the results of a survey for low-frequency radio emission from 17 known exoplanetary systems with the Murchison Widefield Array. This sample includes 13 systems that have not previously been targeted with radio observations. We detected no radio emission at 154 MHz, and put 3τ upper limits in the range 15.2-112.5 mJy on this emission. We also searched for circularly polarized emission and made no detections, obtaining 3τ upper limits in the range 3.4-49.9 mJy. These are comparable with the best low-frequency radio limits in the existing literature and translate to luminosity limits of between 1.2 × 1014 and 1.4 × 1017 Wif the emission is assumed to be 100 per cent circularly polarized. These are the first results from a larger program to systematically search for exoplanetary emission with the MWA.
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