2019
DOI: 10.1109/access.2019.2933387
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DM-Free Curvelet Based Denoising for Astronomical Single Pulse Detection

Abstract: Rotating radio transients (RRATs) are sporadically emitting pulsars which are detected only through single pulse search. Detecting these single pulses in RRATs observation with high detection accuracy is a challenge due to the background noise. It is better to conduct the single pulse detection directly on the raw time-frequency observation than on the de-dispersed data, because de-dispersion process takes very intensive computation. In this paper, we propose to accomplish this idea by treating twodimensional … Show more

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Cited by 4 publications
(7 citation statements)
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References 31 publications
(35 reference statements)
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“…When the input is cartesian arrays such as an image of the form f[],t1t2, 0 t1,t2p, where t 1 , t 2 , and p are real numbers then digital curvelet transforms using three parameters scale, rotation angles and translation parameter can be defined as 30 : cvtD()j,l,normalζ=0t1,t2pf[],t1t2trueψj,l,normalζD[],t1t2¯. …”
Section: Methodsmentioning
confidence: 99%
See 2 more Smart Citations
“…When the input is cartesian arrays such as an image of the form f[],t1t2, 0 t1,t2p, where t 1 , t 2 , and p are real numbers then digital curvelet transforms using three parameters scale, rotation angles and translation parameter can be defined as 30 : cvtD()j,l,normalζ=0t1,t2pf[],t1t2trueψj,l,normalζD[],t1t2¯. …”
Section: Methodsmentioning
confidence: 99%
“…Jean‐Luc et al 19 proposes curvelet‐based multiscale denoising using non‐local means and guided image filter. In the two‐dimensional (2D) domain ℝ2, all curvelets at scale 2‐ j are found by rotation and translations of mother curvelet ψ j with different parameters 30 . Curvelets are defined at scale 2‐ j , orientation θ l and position xζj,l in Equation (). ψj,l,normalζ()x=ψj()Rnormalθl()xxζj,l, where position xζj,l=Rnormalθl1(),ζ1.2jζ2·2j2, Rθ is rotation by θ radians and Rθ1 is its inverse.…”
Section: Methodsmentioning
confidence: 99%
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“…The approach there uses time-frequency images of the data as input to a neural network classifier, which can detect the RFI. An alternative machine learning approach is a support vector machine, which is applied in [14] to recognize transients from features also extracted from a time-frequency representation. Reference [15] describes the application of two types of neural networks for RFI detection.…”
Section: Overview Of State-of-the-artmentioning
confidence: 99%
“…The latter have also been studied in a CMB framework by Vafaei Sadr et al ( 2017) and Hergt et al (2017), using the curvelet transform, while Laliberte et al (2018) use ridgelets to that end within N-body simulations. Gallagher et al (2011) apply both to solar astrophysics, and Jiang et al (2019) use curvelets for radio transient detection.…”
Section: Des Ridges and Curvelet Comparisonmentioning
confidence: 99%