Dhillon, V.S. orcid.org/0000-0003-4236-9642, Marsh, T.R. and Littlefair, S.P. orcid.org/0000-0001-7221-855X (2006) A search for optical bursts from the rotating radio transient J1819-1458 with ULTRACAM. Monthly Notices of the Royal Astronomical Society, 372 (1). pp. 209-212. ISSN 0035-8711
Abstract
We report on the search for optical bursts from J1819−1458, a member of the recently discovered rotating radio transients (RRATs). J1819−1458 exhibits 3-ms bursts with a peak flux of f1.4 GHzν= 3.6 Jy every ∼3.4 min, implying that it is visible for only ∼1 s per day at radio wavelengths. Assuming that the optical light behaves in a similar manner, the most-sensitive way of detecting RRATs is hence not to take long exposures of the field, but instead to capture individual bursts using a high-speed camera mounted on a large-aperture telescope. Using ULTRACAM on the 4.2-m William Herschel Telescope (WHT), we obtained 97 100 images of the field of J1819−1458, each of 18.1 ms exposure time and with essentially no dead-time between the frames. We find no evidence for bursts in u′, g′ and i′ at magnitudes brighter than 15.1, 17.4 and 16.6 (5σ), corresponding to fluxes of less than 3.3, 0.4 and 0.8 mJy at 3560, 4820 and 7610 Å, respectively.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2006 The Authors. Reproduced in accordance with the publisher's self-archiving policy. |
Keywords: | stars: neutron; pulsars: individual: J1819−1458 |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield) |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 10 Apr 2019 13:12 |
Last Modified: | 10 Apr 2019 13:12 |
Status: | Published |
Publisher: | Oxford University Press |
Refereed: | Yes |
Identification Number: | 10.1111/j.1365-2966.2006.10827.x |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:144705 |