output
20022019
most citedObservation of electron-antineutrino disappearance at Daya Bay

2.2k citations

Showing astro-ph.HEShow all

30 papers · 1 filter

astro-ph.HE201942 cited

A deep X-ray view of the bare AGN Ark120. V. Spin determination from disc-Comptonisation efficiency method

D. Porquet, C. Done, J. N. Reeves +13

[Abridged] In our previous work on Ark 120, we found that its 2014 X-ray spectrum is dominated by Comptonisation, while the relativistic reflection emission only originates at tens…

astro-ph.HE201915 cited

Inverse Compton emission from millisecond pulsars in the Galactic bulge

Deheng Song, Oscar Macias, Shunsaku Horiuchi

Analyses of Fermi Gamma-Ray Space Telescope data have revealed a source of excess diffuse gamma rays towards the Galactic center that extends up to roughly 20 degrees in latit…

astro-ph.HE2019159 cited

New Constraints on Sterile Neutrino Dark Matter from M31 Observations

Kenny C. Y. Ng, Brandon M. Roach, Kerstin Perez +4

We use a combined 1.2 Ms of observations of M31 to search for X-ray lines from sterile neutrino dark matter decay. For the first time in a analysis, we consistent…

astro-ph.HE201731 cited

Robust measurement of supernova spectra with future neutrino detectors

Alex Nikrant, Ranjan Laha, Shunsaku Horiuchi

Measuring precise all-flavor neutrino information from a supernova is crucial for understanding the core-collapse process as well as neutrino properties. We apply a chi-squared ana…

astro-ph.HE201717 cited

Multi-wavelength campaign on NGC7469 II. Column densities and variability in the X-ray spectrum

U. Peretz, E. Behar, G. A. Kriss +16

We investigate the ionic column density variability of the ionized outflows associated with NGC7469, to estimate their location and power. This could allow a better understan…

astro-ph.HE201718 cited

Estimating the core compactness of massive stars with Galactic supernova neutrinos

Shunsaku Horiuchi, Ko Nakamura, Tomoya Takiwaki +1

We suggest the future detection of neutrinos from a Galactic core-collapse supernova can be used to infer the progenitor's inner mass density structure. We present the results from…