25 citations · 89 across the 17 of their papers we have counts for
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Fermi bubbles detected in 100 TeV neutrinos
Uri Keshet, Ilya Gurwich
The Fermi bubbles have been identified as a collimated bipolar outflow emanating from the Milky-Way center, tracing strong forward shocks which extend kpc from the Galacti…
Fermi-bubble bulk and edge analysis reveals dust, cooling breaks, and cosmic-ray diffusion, facilitating a self-consistent model
Uri Keshet, Ilya Gurwich, Assaf Lavi +2
The full, radio to -ray spectrum of the Fermi bubbles is shown to be consistent with standard strong-shock electron acceleration at the bubble edge, without the unnatural energy…
Fermi bubbles: the collimated outburst needed to explain forward-shock edges
Santanu Mondal, Uri Keshet, Kartick C. Sarkar +1
The bipolar, nonthermal, high-latitude lobes known as the Fermi bubbles (FBs) are thought to originate from a massive energy release near the Galactic centre (GC). We constrain the…
IceCube constraints on the Fermi Bubbles
Nimrod Sherf, Uri Keshet, Ilya Gurwich
We analyze the IceCube four-year neutrino data in search of a signal from the Fermi bubbles. No signal is found from the bubbles or from their dense shell, even when taking into ac…
Fermi bubbles: high latitude X-ray supersonic shell
Uri Keshet, Ilya Gurwich
The nature of the bipolar, -ray Fermi bubbles (FB) is still unclear, in part because their faint, high-latitude X-ray counterpart has until now eluded a clear detection. We stac…
Fermi bubble edges: spectrum and diffusion function
Uri Keshet, Ilya Gurwich
Current measurements of the -ray Fermi bubbles (FB) are based on model-dependent tracers, carry substantial systematic uncertainties, and are at some tension with each other. We…