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We also added FRB 20171020A among the hosts of the one-off FRBs (blue square) which anyway still is a putative host.Next Article in Journal Testing Quantum Mechanics with an Ultra-Cold Particle Trap.Next Article in Special Issue Probing the Universe with Fast Radio Bursts.Previous Article in Journal The Emerging Reality from Hidden Spaces.
Previous Article in Special Issue Emission Mechanisms of Fast Radio Bursts. Please note that many of the page functionalities wont work as expected without javascript enabled. International Journal of Environmental Research and Public Health (IJERPH). International Journal of Turbomachinery, Propulsion and Power (IJTPP). Journal of Open Innovation: Technology, Market, and Complexity (JOItmC). Journal of Otorhinolaryngology, Hearing and Balance Medicine (OHBM). Journal of Theoretical and Applied Electronic Commerce Research (JTAER). Find support for a specific problem in the support section of our website. Visit our dedicated information section to learn more about MDPI. Received: 24 February 2021 Revised: 10 March 2021 Accepted: 11 March 2021 Published: 23 March 2021. The red circle and the blue ellipse denote the half-light radius of the bright knot and of the extended diffuse emission, respectively. SFR and stellar mass values to derive the specific SFR are from 37, 38 (FRB 20180916B), 93 (FRB 20200120), 78 (FRB 20180924B), 79 (FRB 20190523A). For the two latter FRBs the reported SFR values mark the upper limits (UL). The FRB hosts are indicated by filled squares (green for the one-off, purple for the repeaters) and filled green triangles for the two UL values. The associated errors are smaller than the size of the symbols. The two hosts with the highest masses among the repeaters are the Milky Way, hosting FRB 20200428ASGR J19352154 (framed purple square), and M 81, likely hosting FRB 20200120E, respectively.
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