Second-order transport, quasinormal modes and zero-viscosity limit in the Gauss-Bonnet holographic fluid

(2016)

Authors:

Sašo Grozdanov, Andrei O Starinets

Small Vacuum Energy from Small Equivalence Violation in Scalar Gravity

(2016)

Authors:

Prateek Agrawal, Raman Sundrum

Stellar cooling bounds on new light particles: plasma mixing effects

ArXiv 1611.05852 (2016)

Authors:

Edward Hardy, Robert Lasenby

Transverse oscillations in a coronal loop triggered by a jet

(2016)

Authors:

S Sarkar, V Pant, AK Srivastava, D Banerjee

Very high-energy gamma-ray follow-up program using neutrino triggers from IceCube

Journal of Instrumentation Institute of Physics 11:11 (2016) P11009

Authors:

MG Aartsen, K Abraham, M Ackermann, Subir Sarkar

Abstract:

We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescopes (MAGIC and VERITAS). While IceCube is capable of monitoring the whole sky continuously, high-energy gamma-ray telescopes have restricted fields of view and in general are unlikely to be observing a potential neutrino-flaring source at the time such neutrinos are recorded. The use of neutrino-triggered alerts thus aims at increasing the availability of simultaneous multi-messenger data during potential neutrino flaring activity, which can increase the discovery potential and constrain the phenomenological interpretation of the high-energy emission of selected source classes (e.g. blazars). The requirements of a fast and stable online analysis of potential neutrino signals and its operation are presented, along with first results of the program operating between 14 March 2012 and 31 December 2015.