A detailed radio study of the energetic, nearby, and puzzling GRB 171010A
Monthly Notices of the Royal Astronomical Society Oxford University Press 486:2 (2019) 2721-2729
Abstract:
We present the results of an intensive multi-epoch radio frequency campaign on the energetic and nearby GRB 171010A with the Karl G. Janksy Very Large Array and Arcminute Microkelvin Imager Large Array. We began observing GRB 171010A a day after its initial detection, and were able to monitor the temporal and spectral evolution of the source over the following weeks. The spectra and their evolution are compared to the canonical theories for broad-band GRB afterglows, with which we find a general agreement. There are, however, a number of features that are challenging to explain with a simple forward shock model, and we discuss possible reasons for these discrepancies. This includes the consideration of the existence of a reverse shock component, potential microphysical parameter evolution, and the effect of scintillation.Search for Higgs boson pair production in the b¯bWW∗ decay mode at √s = 13 TeV with the ATLAS detector
Journal of High Energy Physics Springer Berlin Heidelberg 2019:4 (2019) 92
Abstract:
A search for Higgs boson pair production in the b ¯bWW∗ decay mode is performed in the b ¯b`νqq final state using 36.1 fb−1 of proton-proton collision data at a centreof-mass energy of 13 TeV recorded with the ATLAS detector at the Large Hadron Collider. No evidence of events beyond the background expectation is found. Upper limits on the non-resonant pp → HH production cross section of 10 pb and on the resonant production cross section as a function of the HH invariant mass are obtained. Resonant production limits are set for scalar and spin-2 graviton hypotheses in the mass range 500 to 3000 GeV.LinKS: discovering galaxy-scale strong lenses in the Kilo-Degree Survey using convolutional neural networks
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 484:3 (2019) 3879-3896
What do astronomers want from the STFC?
Astronomy and Geophysics Oxford University Press 60:2 (2019) 2.13-2.17
Abstract:
Stephen Serjeant and the STFC's Astronomy Advisory Panel summarize community responses to its consultation on research priorities, undertaken in November 2018.Catalog of quasars from the Kilo-Degree Survey Data Release 3⋆⋆⋆
Astronomy & Astrophysics EDP Sciences 624 (2019) a13