most citedPolarization properties of FRB 20201124A from detections with the 100-m Effelsberg Radio Telescope

75 citations · 176 across the 4 of their papers we have counts for

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6 papers

astro-ph.HE202125 cited

Burst properties of the highly active FRB 20201124A using uGMRT

V. R. Marthi, S. Bethapudi, R. A. Main +7

We report the observations of the highly active FRb20201124A with the upgraded Giant Metrewave Radio Telescope at 550-750~MHz. These observations in the incoherent array mode simul…

astro-ph.HE202175 cited

Polarization properties of FRB 20201124A from detections with the 100-m Effelsberg Radio Telescope

G. H. Hilmarsson, L. G. Spitler, R. A. Main +1

The repeating FRB source, FRB 20201124A, was found to be highly active in March and April 2021. We observed the source with the Effelsberg 100-m radio telescope at 1.36 GHz on 9 Ap…

astro-ph.HE202010 cited

Observing superluminous supernovae and long gamma ray bursts as potential birthplaces of repeating fast radio bursts

G. H. Hilmarsson, L. G. Spitler, E. F. Keane +12

Superluminous supernovae (SLSNe) and long gamma ray bursts (LGRBs) have been proposed as progenitors of repeating Fast Radio Bursts (FRBs). In this scenario, bursts originate from…

astro-ph.HE2020

Rotation Measure Evolution of the Repeating Fast Radio Burst Source FRB 121102

G. H. Hilmarsson, D. Michilli, L. G. Spitler +10

The repeating fast radio burst source FRB 121102 has been shown to have an exceptionally high and variable Faraday rotation measure (RM), which must be imparted within its host gal…

astro-ph.HE2020

Repeating behaviour of FRB 121102: periodicity, waiting times and energy distribution

M. Cruces, L. G. Spitler, P. Scholz +7

Detections from the repeating fast radio burst FRB 121102 are clustered in time, noticeable even in the earliest repeat bursts. Recently, it was argued that the source activity is…

astro-ph.HE202066 cited

Simultaneous multi-telescope observations of FRB 121102

M. Caleb, B. W. Stappers, T. D. Abbott +29

We present 11 detections of FRB 121102 in ~3 hours of observations during its 'active' period on the 10th of September 2019. The detections were made using the newly deployed MeerT…