摘要: Multi-element interferometers such as MeerKAT, which observe with high time
resolution and have a wide field-of-view, provide an ideal opportunity to
perform real-time, untargeted transient and pulsar searches. However, because
of data storage limitations, it is not always feasible to store the baseband
data required to image the field of a discovered transient or pulsar. This
limits the ability of surveys to effectively localise their discoveries and may
restrict opportunities for follow-up science, especially of one-off events like
some Fast Radio Bursts (FRBs). Here we present a novel maximum-likelihood
estimation approach to localising transients and pulsars detected in multiple
MeerKAT tied-array beams at once, which we call Tied Array Beam Localisation
(TABLo), as well as a Python implementation of the method named SeeKAT. We
provide real-world examples of SeeKAT's use as well as a Monte Carlo analysis
to show that it is capable of localising single pulses detected in beamformed
MeerKAT data to (sub-)arcsecond precision.
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分类:
天文学
>>
天文学
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引用:
ChinaXiv:202303.02604
(或此版本
ChinaXiv:202303.02604V1)
DOI:10.12074/202303.02604V1
CSTR:32003.36.ChinaXiv.202303.02604.V1
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科创链TXID:
41f38d12-4e59-46bb-841a-c7d29d4f18b5
- 推荐引用方式:
M. C. Bezuidenhout,C. J. Clark,R. P. Breton,B. W. Stappers,E. D. Barr,M. Caleb,W. Chen,F. Jankowski,M. Kramer,K. Rajwade,M. Surnis.Tied-Array Beam Localisation of Radio Transients and Pulsars.null.[ChinaXiv:202303.02604V1]
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