Murchison widefield array observations of anomalous variability: A serendipitous night-time detection of interplanetary scintillation
MetadataShow full item record
We present observations of high-amplitude rapid (2 s) variability toward two bright, compact extragalactic radio sources out of several hundred of the brightest radio sources in one of the Murchison Widefield Array (MWA) Epoch of Reionization fields using the MWA at 155 MHz. After rejecting intrinsic, instrumental, and ionospheric origins we consider the most likely explanation for this variability to be interplanetary scintillation (IPS), likely the result of a large coronal mass ejection propagating from the Sun. This is confirmed by roughly contemporaneous observations with the Ooty Radio Telescope. We see evidence for structure on spatial scales ranging from <1000 to > 10 6 km. The serendipitous night-time nature of these detections illustrates the new regime that the MWA has opened for IPS studies with sensitive night-time, wide-field, low-frequency observations. This regime complements traditional dedicated strategies for observing IPS and can be utilized in real-time to facilitate dedicated follow-up observations. At the same time, it allows large-scale surveys for compact (arcsec) structures in low-frequency radio sources despite the resolution of the array.
This is an author-created, un-copy edited version of an article accepted for publication in Astrophysical Journal Letters. The publisher is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at http://doi.org/10.1088/2041-8205/809/1/L12
Showing items related by title, author, creator and subject.
Jones, S.; McHardy, I.; Moss, D.; Seymour, Nick; Breedt, E.; Uttley, P.; Körding, E.; Tudose, V. (2011)We present intensive quasi-simultaneous X-ray and radio monitoring of the narrow line Seyfert 1 galaxy NGC 4051, over a 16-month period in 2000–01. The X-ray observations were made with the Proportional Counter Array on ...
The Low-Frequency Environment of the Murchison Widefield Array: Radio-Frequency Interference Analysis and MitigationOffringa, A.; Wayth, Randall; Hurley-Walker, N.; Kaplan, D.; Barry, N.; Beardsley, A.; Bell, M.; Bernardi, G.; Bowman, J.; Briggs, F.; Callingham, J.; Cappallo, R.; Carroll, P.; Deshpande, A.; Dillon, J.; Dwarakanath, K.; Ewall-Wice, A.; Feng, L.; For, B.; Gaensler, B.; Greenhill, L.; Hancock, P.; Hazelton, B.; Hewitt, J.; Hindson, L.; Jacobs, D.; Johnston-Hollitt, M.; Kapinska, A.; Kim, H.; Kittiwisit, P.; Lenc, E.; Line, J.; Loeb, A.; Lonsdale, C.; McKinley, B.; McWhirter, S.; Mitchell, D.; Morales, M.; Morgan, E.; Morgan, J.; Neben, A.; Oberoi, D.; Ord, Stephen; Paul, S.; Pindor, B.; Pober, J.; Prabu, T.; Procopio, P.; Riding, J.; Shankar, N.; Sethi, S.; Srivani, K.; Staveley-Smith, L.; Subrahmanyan, R.; Sullivan, I.; Tegmark, M.; Thyagarajan, N.; Tingay, Steven; Trott, C.; Webster, R.; Williams, A.; Williams, C.; Wu, C.; Wyithe, J.; Zheng, Q. (2015)The Murchison Widefield Array is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array. We describe the automated radio-frequency ...
Anderson, Gemma; Staley, T.; van der Horst, A.; Fender, R.; Rowlinson, A.; Mooley, K.; Broderick, J.; Wijers, R.; Rumsey, C.; Titterington, D. (2018)We present the Arcminute Microkelvin Imager (AMI) Large Array catalogue of 139 gamma-ray bursts (GRBs). AMI observes at a central frequency of 15.7 GHz and is equipped with a fully automated rapid-response mode, which ...