works on

From the 1 of 1.2k papers with an AI index.

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20022025
most citedObservation of electron-antineutrino disappearance at Daya Bay

2.2k citations

Showing 2017 · astro-ph.HEShow all

11 papers · 2 filters

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…

astro-ph.HE201753 cited

NuSTAR Resolves the First Dual AGN above 10 keV in SWIFT J2028.5+2543

Michael J. Koss, Ana Glidden, Mislav Balokovic +19

We have discovered heavy obscuration in the dual active galactic nucleus (AGN) in the Swift/Burst Alert Telescope (BAT) source SWIFT J2028.5+2543 using Nuclear Spectroscopic Telesc…

astro-ph.HE201799 cited

A deep X-ray view of the bare AGN Ark120. IV. XMM-Newton and NuSTAR spectra dominated by two temperature (warm, hot) Comptonization processes

D. Porquet, J. N. Reeves, G. Matt +16

We perform an X-ray spectral analysis of the brightest and cleanest bare AGN known so far, Ark 120, in order to determine the process(es) at work in the vicinity of the SMBH. We pr…

astro-ph.HE201793 cited

Chasing obscuration in type-I AGN: discovery of an eclipsing clumpy wind at the outer broad-line region of NGC 3783

M. Mehdipour, J. S. Kaastra, G. A. Kriss +21

In 2016 we carried out a Swift monitoring program to track the X-ray hardness variability of eight type-I AGN over a year. The purpose of this monitoring was to find intense obscur…