activity
20182022
most citedGraph Neural Networks for Low-Energy Event Classification & Reconstruction in IceCube

38 citations · 64 across the 7 of their papers we have counts for

collaborators

8 papers

hep-ex202238 cited

Graph Neural Networks for Low-Energy Event Classification & Reconstruction in IceCube

R. Abbasi, M. Ackermann, J. Adams +380

IceCube, a cubic-kilometer array of optical sensors built to detect atmospheric and astrophysical neutrinos between 1 GeV and 1 PeV, is deployed 1.45 km to 2.45 km below the surfac…

astro-ph.IM2020

An update on the development of ASPIRED

Marco C Lam, Robert J Smith, Josh Veitch-Michaelis +2

We are reporting the updates in version 0.2.0 of the Automated SpectroPhotometric REDuction (ASPIRED) pipeline, designed for common use on different instruments. The default settin…

astro-ph.IM20203 cited

Learnings from Frontier Development Lab and SpaceML -- AI Accelerators for NASA and ESA

Siddha Ganju, Anirudh Koul, Alexander Lavin +3

Research with AI and ML technologies lives in a variety of settings with often asynchronous goals and timelines: academic labs and government organizations pursue open-ended resear…

astro-ph.GA202015 cited

The WAGGS project -- III. Discrepant mass-to-light ratios of Galactic globular clusters at high metallicity

H. Dalgleish, S. Kamann, C. Usher +10

Observed mass-to-light ratios (M/L) of metal-rich globular clusters (GCs) disagree with theoretical predictions. This discrepancy is of fundamental importance since stellar populat…

physics.ed-ph20195 cited

Assessing the influence of one astronomy camp over 50 years

Hannah Dalgleish, Josh Veitch-Michaelis

The International Astronomical Youth Camp has benefited thousands of lives during its 50-year history. We explore the pedagogy behind this success, review a survey taken by more th…

astro-ph.IM20191 cited

RASCAL: Towards automated spectral wavelength calibration

Josh Veitch-Michaelis, Marco C Lam

Wavelength calibration is a routine and critical part of any spectral work-flow, but many astronomers still resort to matching detected peaks and emission lines by hand. We present…