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19952023
most citedOverview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory

1.7k citations · 6.7k across the 100 of their papers we have counts for

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41 papers · 1 filter

astro-ph.GA2023★ 8 cited

The co-evolution of strong AGN and central galaxies in different environments

V. M. Sampaio, A. Aragón-Salamanca, M. R. Merrifield +3

We exploit a sample of 80,000 SDSS central galaxies to investigate the effect of AGN feedback on their evolution. We trace the demographics of optically-selected AGN (Seyferts) as…

astro-ph.GA2021★ 8 cited

Clusters' far-reaching influence on narrow-angle tail radio galaxies

K de Vos, N. A. Hatch, M. R. Merrifield +1

In order to study the ram-pressure interaction between radio galaxies and the intracluster medium, we analyse a sample of 208 highly-bent narrow-angle tail radio sources (NATs) in…

astro-ph.GA2021★ 2 cited

An analytical model to kinematically identify thin discs in MaNGA galaxies

Meng Yang, Anne-Marie Weijmans, Matthew A. Bershady +3

We present an analytical model to identify thin discs in galaxies, and apply this model to a sample of SDSS MaNGA galaxies. This model fits the velocity and velocity dispersion fie…

astro-ph.GA2021

Infrared lags in the light curves of AGN measured using a deep survey

E. Elmer, M. Merrifield, O. Almaini +2

Information on the structure around active galactic nuclei (AGN) has long been derived from measuring lags in their varying light output at different wavelengths. In principle, inf…

astro-ph.GA2021★ 8 cited

Size, shade or shape? The contribution of galaxies of different types to the star-formation history of the Universe from SDSS-IV MaNGA

Thomas Peterken, Alfonso Aragón-Salamanca, Michael Merrifield +7

By fitting stellar populations to SDSS-IV MaNGA survey observations of ~7000 suitably-weighted individual galaxies, we reconstruct the star-formation history of the Universe, which…

astro-ph.GA2021★ 13 cited

SDSS-IV MaNGA: the "G-dwarf problem" revisited

Michael J. Greener, Michael Merrifield, Alfonso Aragón-Salamanca +3

The levels of heavy elements in stars are the product of enhancement by previous stellar generations, and the distribution of this metallicity among the population contains clues t…