activity
20152020
most citedFlavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

197 citations · 260 across the 4 of their papers we have counts for

collaborators

6 papers

physics.ins-det2020

Construction and commissioning of CMS CE prototype silicon modules

B. Acar, G. Adamov, C. Adloff +327

As part of its HL-LHC upgrade program, the CMS Collaboration is developing a High Granularity Calorimeter (CE) to replace the existing endcap calorimeters. The CE is a sampling cal…

physics.ins-det2020

The DAQ system of the 12,000 Channel CMS High Granularity Calorimeter Prototype

B. Acar, G. Adamov, C. Adloff +327

The CMS experiment at the CERN LHC will be upgraded to accommodate the 5-fold increase in the instantaneous luminosity expected at the High-Luminosity LHC (HL-LHC). Concomitant wit…

hep-ex202032 cited

Search for new physics in top quark production with additional leptons in proton-proton collisions at 13 TeV using effective field theory

CMS Collaboration

Events containing one or more top quarks produced with additional prompt leptons are used to search for new physics within the framework of an effective field theory (EFT). The dat…

astro-ph.HE2017

The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part III: Cosmic Rays

IceCube Collaboration, M. G. Aartsen, M. Ackermann +312

Papers on cosmic-ray measurements submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collaboration

astro-ph.HE201631 cited

Lowering IceCube's Energy Threshold for Point Source Searches in the Southern Sky

IceCube Collaboration, M. G. Aartsen, K. Abraham +317

Observation of a point source of astrophysical neutrinos would be a "smoking gun" signature of a cosmic-ray accelerator. While IceCube has recently discovered a diffuse flux of ast…

astro-ph.HE2015197 cited

Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

IceCube Collaboration, M. G. Aartsen, M. Ackermann +300

A diffuse flux of astrophysical neutrinos above has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical f…