AT 2018cow VLBI: no long-lived relativistic outflow
M. F. Bietenholz, E. Berger(Center for Astrophysics Harvard & Smithsonian), D. L. Coppejans(Northwestern University), D. Milisavljević(Harvard University Press), G. Terreran(Las Cumbres Observatory Global Telescope Network), N. Bartel(York University), M. K. Argo(University of Lancashire), K. D. Alexander(University of Arizona), R. Margutti(Harvard University Press), Tarraneh Eftekhari(Northwestern University)
Cited by 33
Related Papers
Beaming in Gamma-Ray Bursts: Evidence for a Standard Energy Reservoir
|The Astrophysical Journal|2001|1.2k
The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
|The Astrophysical Journal Letters|2017|1k
Joint Analysis of BICEP2/<i>Keck Array</i>and<i>Planck</i>Data
|Physical Review Letters|2015|986
Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz Band
|Physical Review Letters|2016|675
A γ-ray burst at a redshift of z ≈ 8.2
|Nature|2009|639