activity
19982023
most citedThe VMC Survey - I. Strategy and First Data

346 citations · 4.4k across the 81 of their papers we have counts for

collaborators

82 papers

astro-ph.SR2023★ 17 cited

A Naive Bayes Classifier for identifying Class II YSOs

Andrew J. Wilson, Ben S. Lakeland, Tom J. Wilson +1

A naive Bayes classifier for identifying Class II YSOs has been constructed and applied to a region of the Northern Galactic Plane containing 8 million sources with good quality Ga…

astro-ph.IM2022★ 211 cited

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Shoko Jin, Scott C. Trager, Gavin B. Dalton +212

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…

astro-ph.IM2022

ABORAS: polarimetric, 10cm/s RV observations of the Sun as a star

Casper Farret Jentink, Annelies Mortier, Frans Snik +4

We present a description of A dual-Beam pOlarimetric Robotic Aperture for the Sun (ABORAS), to serve as a Solar input with a dedicated Stokes V polarimeter for the HARPS3 high-reso…

astro-ph.SR2022★ 12 cited

Towards an understanding of YSO variability: A multi-wavelength analysis of bursting, dipping, and symmetrically varying light curves of disc-bearing YSOs

Ben S. Lakeland, Tim Naylor

Using simultaneous optical and infrared light curves of disc-bearing young stars in NGC 2264, we perform the first multi-wavelength structure function study of YSOs. We find that d…

astro-ph.GA2022★ 4 cited

Observational Bias and Young Massive Cluster Characterisation I. 2D Perspective Effects

Anne S. M. Buckner, Kong You Liow, Clare L. Dobbs +2

Understanding the formation and evolution of high mass star clusters requires comparisons between theoretical and observational data to be made. Unfortunately, while the full phase…

astro-ph.GA2021★ 5 cited

Spatial Statistics in Star Forming Regions: Is Star Formation Driven By Column Density Alone?

Brendan Retter, Jennifer Hatchell, Tim Naylor

Star formation is known to occur more readily where more raw materials are available. This is often expressed by a 'Kennicutt-Schmidt' relation where the surface density of Young S…