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papers

Publications (5)

astro-ph.EP2020

ExoMol line lists -- XL. Ro-vibrational molecular line list for the hydronium ion (H $_{3}$ O $^{+}$ )

S. N. Yurchenko, Jonathan Tennyson, Steve Miller +3

A new line list for hydronium (H $_{3}$ $^{16}$ O $^{+}$ ) is computed. The line list is based on a new ab initio dipole moment surface (CCSD(T)/aug-cc-pVQZ) and a new empirical potential e…

hep-ph2019

The Machine Learning Landscape of Top Taggers

G. Kasieczka, T. Plehn, A. Butter +24

Based on the established task of identifying boosted, hadronically decaying top quarks, we compare a wide range of modern machine learning approaches. Unlike most established metho…

astro-ph.EP2017

The quest for H $_{3}^{+}$ at Neptune: deep burn observations with NASA IRTF iSHELL

H. Melin, L. N. Fletcher, T. S. Stallard +4

Emission from the molecular ion H $_{3}^{+}$ is a powerful diagnostic of the upper atmosphere of Jupiter, Saturn, and Uranus, but it remains undetected at Neptune. In search of this emi…

hep-ph2018

Interpreting top-quark LHC measurements in the standard-model effective field theory

J. A. Aguilar Saavedra, C. Degrande, G. Durieux +32

This note proposes common standards and prescriptions for the effective-field-theory interpretation of top-quark measurements at the LHC.

astro-ph.EP2019

Modelling H $_{3}^{+}$ in planetary atmospheres: effects of vertical gradients on observed quantities

L. Moore, H. Melin, J. O'Donoghue +5

Since its discovery in the aurorae of Jupiter ~30 years ago, the H $_{3}^{+}$ ion has served as an invaluable probe of giant planet upper atmospheres. However, the vast majority of…