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19932026
most citedGW190521: A Binary Black Hole Merger with a Total Mass of

1.3k citations

Showing 2015Show all

20 papers · 1 filter

physics.ins-det2015★ 61 cited

The PROSPECT Physics Program

J. Ashenfelter, B. Balantekin, H. R. Band +61

The Precision Reactor Oscillation and Spectrum Experiment, PROSPECT, is designed to make a precise measurement of the antineutrino spectrum from a highly-enriched uranium reactor a…

astro-ph.GA2015★ 87 cited

Excitation of coupled stellar motions in the Galactic Disk by orbiting satellites

E. D'Onghia, P. Madau, C. Vera-Ciro +2

We use a set of high-resolution N-body simulations of the Galactic disk to study its interactions with the population of satellites predicted cosmologically. One simulation illustr…

astro-ph.HE2015★ 145 cited

Evidence against star-forming galaxies as the dominant source of IceCube neutrinos

Keith Bechtol, Markus Ahlers, Mattia Di Mauro +2

The cumulative emission resulting from hadronic cosmic-ray interactions in star-forming galaxies (SFGs) has been proposed as the dominant contribution to the astrophysical neutrino…

physics.ao-ph2015★ 1 cited

Nonlinear traveling waves for the skeleton of the Madden-Julian oscillation

Shengqian Chen, Samuel N. Stechmann

The Madden-Julian Oscillation (MJO) is the dominant component of intraseasonal (30-90 days) variability in the tropical atmosphere. Here, traveling wave solutions are presented for…

astro-ph.HE2015★ 48 cited

Turbulent Reconnection in Relativistic Plasmas And Effects of Compressibility

Makoto Takamoto, Tsuyoshi Inoue, Alexandre Lazarian

We report turbulence effects on magnetic reconnection in relativistic plasmas using 3-dimensional relativistic resistive magnetohydrodynamics simulations. We found reconnection rat…

astro-ph.GA2015

CARMA CO Observations of Three Extremely Metal-Poor, Star-Forming Galaxies

Steven R. Warren, Edward Molter, John M. Cannon +11

We present sensitive CO (J = 1 - 0) emission line observations of three metal-poor dwarf irregular galaxies Leo P (Z ~ 3% Z_Solar), Sextans A (Z ~ 7.5% Z_Solar), and Sextans B (Z ~…