Low frequency view of GRB 190114C reveals time varying shock micro-physics

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Low frequency view of GRB 190114C reveals time varying shock micro-physics

We present radio and optical afterglow observations of the TeV-bright long gamma-ray burst 190114C at a redshift of z = 0.425, which was detected by the Major Atmospheric Gamma Imaging Cherenkov telescope. Our observations with Atacama Large Millimeter/submillitmeter Array, Australia Telescope Compa...

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Bibliographic Details
Main Authors:	Misra, K., Resmi, L., Kann, D.A., Marongiu, M., Moin, A., Klose, S., Bernardi, G., Postigo, A.D.U., Jaiswal, V.K., Schulze, S., Perley, D.A., Ghosh, A., Dimple, D., Kumar, H., Gupta, R., Michałowski, M.J., Martín, S., Cockeram, A., Cherukuri, S.V., Bhalerao, V., Anderson, Gemma, Pandey, S.B., Anupama, G.C., Thöne, C.C., Barway, S., Wieringa, M.H., Fynbo, J.P.U., Habeeb, N.
Format:	Journal Article
Language:	English
Published:	OXFORD UNIV PRESS 2021
Subjects:	Science & Technology Physical Sciences Astronomy & Astrophysics gamma-ray burst general-gamma-ray burst individual-GRB 190114C radio observations GAMMA-RAY-BURST AFTERGLOW LIGHT CURVES HIGH-ENERGY EMISSION REVERSE SHOCK SWIFT-ERA PRE-SWIFT OPTICAL AFTERGLOW RADIO AFTERGLOW SCINTILLATION SYNCHROTRON
Online Access:	http://purl.org/au-research/grants/arc/DE180100346 http://hdl.handle.net/20.500.11937/90305

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