| Autor: |
D. R. Madison, D. Agarwal, K. Aggarwal, O. Young, H. T. Cromartie, M. T. Lam, S. Chatterjee, J. M. Cordes, N. Garver-Daniels, D. R. Lorimer, R. S. Lynch, M. A. McLaughlin, S. M. Ransom, R. S. Wharton |
| Předmět: |
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| Zdroj: |
Astrophysical Journal; 12/20/2019, Vol. 887 Issue 2, p1-1, 1p |
| Abstrakt: |
Some short gamma-ray bursts (SGRBs) are thought to be caused by the mergers of binary neutron stars which may sometimes produce massive neutron star remnants capable of producing extragalactic fast radio bursts (FRBs). We conducted a deep search for FRBs from the sites of six low-redshift SGRBs. We collected high time- and frequency-resolution data from each of the sites for 10 hr using the 2 GHz receiver of the Green Bank Telescope (GBT). Two of the SGRB sites we targeted were visible with the Arecibo Radio Telescope with which we conducted an additional 10 hr of 1.4 GHz observations for each. We searched our data for FRBs using the GPU-optimized dedispersion algorithm heimdall and the machine-learning-based package Fast Extragalactic Transient Candidate Hunter. We did not discover any FRBs, but would have detected any with peak flux densities in excess of 87 mJy at the GBT or 21 mJy at Arecibo with a signal-to-noise ratio of at least 10. The isotropic-equivalent energy of any FRBs emitted from these sites in our bands during our observations must not have exceeded a few times 1038 erg, comparable to some of the lowest energy bursts yet seen from the first known repeating FRB 121102. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
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