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Dust reddening and extinction curves towards gamma-ray bursts at z > 4
Jan Bolmer, Jochen Greiner, Thomas Krühler +4
Dust is known to be produced in the envelopes of AGB stars, the expanded shells of supernova (SN) remnants, and in situ grain growth in the ISM, although the corresponding efficien…
Spatially resolved MaNGA observations of the host galaxy of superluminous supernova 2017egm
Ting-Wan Chen, Patricia Schady, Lin Xiao +6
Superluminous supernovae (SLSNe) are found predominantly in dwarf galaxies, indicating that their progenitors have a low metallicity. However, the most nearby SLSN to date, SN 2017…
The environment of the SN-less GRB 111005A at z = 0.0133
M. Tanga, T. Krühler, P. Schady +5
The collapsar model has proved highly successful in explaining the properties of long gamma-ray bursts (GRBs), with the most direct confirmation being the detection of a supernova…
Gamma-ray bursts and their use as cosmic probes
Patricia Schady
Since the launch of the highly successful and ongoing Swift mission, the field of gamma-ray bursts (GRBs) has undergone a revolution. The arcsecond GRB localizations available with…
Gas inflow and outflow in an interacting high-redshift galaxy: The remarkable host environment of GRB 080810 at
P. Wiseman, D. A. Perley, P. Schady +5
We reveal multiple components of an interacting galaxy system at through a detailed analysis of the exquisite high-resolution Keck/HIRES spectrum of the afterglow of…
Hot gas around SN 1998bw: Inferring the progenitor from its environment
Thomas Krühler, Hanindyo Kuncarayakti, Patricia Schady +3
Spatially-resolved spectroscopy of the environments of explosive transients carries detailed information about the physical properties of the stellar population that gave rise to t…