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CHIME/FRB Detection of the Original Repeating Fast Radio Burst Source FRB 121102

  • Authors: A. Josephy, P. Chawla, E. Fonseca, C. Ng, C. Patel, Z. Pleunis, P. Scholz, B. C. Andersen, K. Bandura, M. Bhardwaj, M. M. Boyce, P. J. Boyle, C. Brar, D. Cubranic, M. Dobbs, B. M. Gaensler, A. Gill, U. Giri, D. C. Good, M. Halpern, G. Hinshaw, V. M. Kaspi, T. L. Landecker, D. A. Lang, H.-H. Lin, K. W. Masui, R. Mckinven, J. Mena-Parra, M. Merryfield, D. Michilli, N. Milutinovic, A. Naidu, U. Pen, M. Rafiei-Ravandi, M. Rahman, S. M. Ransom, A. Renard, S. R. Siegel, K. M. Smith, I. H. Stairs, S. P. Tendulkar, K. Vanderlinde, P. Yadav, and A. V. Zwaniga

2019 The Astrophysical Journal Letters 882 L18.

  • Provider: AAS Journals

Caption: Figure 4.

Structure-optimizing DM method. The main panel shows the signed square (n = 2) of the forward time derivative of the smoothed DM transform (DMT), where the color scale reflects the local steepness of frequency-averaged burst profiles for different DMs. While absolute values are taken for the final metric, we show the sign to highlight rising and falling regions. Likewise, we show n = 2 to highlight structure beyond a singular sharp rise. The curves in the right panel are high-order polynomial fits to time-averaged time derivatives to the power n, normalized to DM 563.6 pc cm−3. Dashed lines correspond to the DMs used to produce the six frequency-averaged burst profiles at the top, with the structure-optimizing DM indicated in bold. Note that the profiles have been convolved with a 3 ms boxcar to match the smoothing used on the DM transform prior to taking the time derivative.

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