activity
19972024
most citedThe GALAH Survey: Scientific Motivation

839 citations · 24.6k across the 409 of their papers we have counts for

collaborators

410 papers

astro-ph.CO2024★ 3 cited

Free-floating "planets'' in the macrolensed quasar Q2237+0305

Artem Tuntsov, Geraint Lewis, Mark Walker

It has been claimed that the variability of field quasars resembles gravitational lensing by a large cosmological population of free-floating planets with mass of about 10 Earths.…

astro-ph.CO2023

The Redshift Difference in Gravitational Lensed Systems: A Novel Probe of Cosmology

Chengyi Wang, Krzysztof Bolejko, Geraint F. Lewis

The exploration of the redshift drift, a direct measurement of cosmological expansion, is expected to take several decades of observation with stable, sensitive instruments. We int…

astro-ph.GA2023★ 1 cited

RomAndromeda: The Roman Survey of the Andromeda Halo

Arjun Dey, Joan Najita, Carrie Filion +50

As our nearest large neighbor, the Andromeda Galaxy provides a unique laboratory for investigating galaxy formation and the distribution and substructure properties of dark matter…

astro-ph.CO2023★ 2 cited

Detection of the Cosmological Time Dilation of High Redshift Quasars

Geraint F. Lewis, Brendon J. Brewer

A fundamental prediction of relativistic cosmologies is that, due to the expansion of space, observations of the distant cosmos should be time dilated and appear to run slower than…

astro-ph.CO2023★ 8 cited

Testing the Cosmological Principle: On the Time Dilation of Distant Sources

Oliver T. Oayda, Geraint F. Lewis

We present a novel test of the cosmological principle: the idea that, on sufficiently large scales, the universe should appear homogeneous and isotropic to observers comoving with…

astro-ph.GA2023★ 11 cited

The GALAH survey: New diffuse interstellar bands found in residuals of 872,000 stellar spectra

Rok Vogrinčič, Janez Kos, Tomaž Zwitter +11

We use more than 872,000 mid-to-high resolution (R 20,000) spectra of stars from the GALAH survey to discern the spectra of diffuse interstellar bands (DIBs). We use four wi…