tipa -- 11/19/2015

Are we there yet? Time to detection of nanohertz gravitational waves based on pulsar-timing array limits

• S. R. Taylor, M. Vallisneri, J. A. Ellis, C. M. F. Mingarelli, T. J. W. Lazio, R. van Haasteren

Standing Shock Instability in Advection-Dominated Accretion Flows

• Truong Le, Kent S. Wood, Michael T. Wolff, Peter A. Becker, Joy Putney

Sodium Absorption Systems towards SN Ia 2014J Originate on Interstellar Scales

• K. Maeda, A. Tajitsu, K.S. Kawabata, R. Foley, S. Honda, Y. Moritani, M. Tanaka, O. Hashimoto, M. Ishigaki, J.D. Simon, M.M.Phillips, M. Yamanaka, D. Nogami, A. Arai, W. Aoki, K. Nomoto, D. Milisavljevic, P.A. Mazzali, A.M. Soderberg, M. Schramm, B. Sato, H. Harakawa, N. Morrell, N. Arimoto

Collisions between Dark Matter Confined High Velocity Clouds and Magnetized Galactic Disks: The Smith Cloud

• Jason Galyardt, Robin L. Shelton

Comparison of Hipparcos Trigonometric and Mount Wilson Spectroscopic Parallaxes for 90 Subgiants that Defined the Class in 1935

• Allan Sandage, Rachael L. Beaton, Steven R. Majewski

Observation of Energy and Baseline Dependent Reactor Antineutrino Disappearance in the RENO Experiment

• RENO Collaboration

Identification of nuclear effects in neutrino-carbon interactions at low three-momentum transfer

• MINERvA Collaboration