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20112024
most citedRadio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection

138 citations · 204 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2024

Radio Galaxy Zoo Data Release 1: 100,185 radio source classifications from the FIRST and ATLAS surveys

O. Ivy Wong, A. F. Garon, M. J. Alger +15

Radio galaxies can extend far beyond the stellar component of their originating host galaxies, and their radio emission can consist of multiple discrete components. Furthermore, th…

astro-ph.GA2022★ 16 cited

Evidence for non-merger co-evolution of galaxies and their supermassive black holes

R. J. Smethurst, R. S. Beckmann, B. D. Simmons +7

Recent observational and theoretical studies have suggested that supermassive black holes (SMBHs) grow mostly through non-merger (`secular') processes. Since galaxy mergers lead to…

astro-ph.GA2022★ 14 cited

Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy

R. S. Beckmann, R. J. Smethurst, B. D. Simmons +7

Here we use the Horizon-AGN simulation to test whether the spins of SMBHs in merger-free galaxies are higher. We select samples using an observationally motivated bulge-to-total ma…

astro-ph.GA2015★ 138 cited

Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection

J. K. Banfield, O. I. Wong, K. W. Willett +33

We present results from the first twelve months of operation of Radio Galaxy Zoo, which upon completion will enable visual inspection of over 170,000 radio sources to determine the…

astro-ph.CO2011★ 36 cited

Obscured GOODS AGN and Their Host Galaxies at z < 1.25: The Slow Black Hole Growth Phase

B. D. Simmons, J. Van Duyne, C. M. Urry +4

We compute black hole masses and bolometric luminosities for 87 obscured AGN in the redshift range 0.25 < z < 1.25, selected from the GOODS deep multi-wavelength survey fields via…