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20182026
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astro-ph.GA2026

Classifying Quasar Types Without a Spectrum

Adrien Hélias, Pauline Barmby, Sarah C. Gallagher +2

Distinguishing between Type 1 and Type 2 quasars is important because it helps us understand accretion regimes, black hole mass scaling, disk instabilities and feedback processes i…

astro-ph.GA2025

Investigating the AGN variability timescale -- black hole mass relationship with Gaia, SDSS and ZTF

Adrien Hélias, Sarah C. Gallagher, Pauline Barmby

Active galactic nuclei (AGNs) exhibit variability in their luminosities with timescales that correlate with the mass of the black hole at the centre of the AGN. Presently, the empi…

astro-ph.GA2025

AGN--Host Galaxy Image Decomposition with JWST

Callum Dewsnap, Pauline Barmby, Sarah C. Gallagher

The ability to disentangle the light of an AGN from its host galaxy is strongly dependent on the spatial resolution and depth of the imaging. As the capabilities of imaging systems…

astro-ph.GA2025

TONGS: A Treasury Of Nearby Galaxy Surveys

Hannah S. Christie, Adrien Hélias, Matheus do Carmo Carvalho +1

The beginning of the 21st century marked the "modern era of galaxy surveys" in astronomy. Rapid innovation in observing technology, combined with the base built by galaxy catalogs…

astro-ph.GA2024

Comparing Gaia, NED and SIMBAD source classifications in nearby galaxies

J. Hales, P. Barmby

Gaia Data Release 3 (DR3) provides the first classifications for the sources in Gaia's all-sky database. Most Gaia sources are stars in the Milky Way, but DR3 also contains many so…

astro-ph.GA2018

Deconstructing a galaxy: colour distributions of point sources in Messier 83

A. Kiar, P. Barmby, A. Hidalgo

What do we see when we look at a nearby, well-resolved galaxy? Thousands of individual sources are detected in multiband imaging observations of even a fraction of a nearby galaxy,…