Published November 16, 2019
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Time-slide correlation analysis of post-merger Extended Emission to GW170817
Description
Nico van Kampen Colloquium, ITP, Utrecht (October 23 2019, https://zenodo.org/record/3528005) - Movie clip. Shown is the result of $\chi$-image analysis of merged (H1,L1)-spectrograms produced in time-slide correlation analysis of H1-L1 data of GW170817. Time-sliding over -32s $\le \Delta t \le 32$s, including one-sample steps around the zero-crossing $\Delta t = 0$, reveals clustering of $\chi$-peak values representing a correlated (H1,L1)-detector response to a gravitational-wave signal.
Notes
Preferred citation: Central engine of GRB170817A: Neutron star versus Kerr black hole based on multimessenger calorimetry and event timing, Maurice H. P. M. van Putten, Massimo Della Valle A&A 669 A36 (2023), DOI: 10.1051/0004-6361/202142974
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Related works
- Is cited by
- Journal article: 10.1051/0004-6361/202142974 (DOI)
- Is part of
- Presentation: https://zenodo.org/record/3528005 (URL)