activity
20112026
most citedThe Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment

681 citations · 4.2k across the 111 of their papers we have counts for

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Showing 2022Show all

8 papers · 1 filter

astro-ph.GA2022★ 22 cited

The galaxy mass-size relation in CARLA clusters and proto-clusters at 1.4 < z < 2.8: larger cluster galaxy sizes

Anton V. Afanasiev, Simona Mei, Hao Fu +12

(Abridged) We study the galaxy mass-size relation in CARLA spectroscopically confirmed clusters at , which span a total stellar mass $11.3<\mathrm{log}(M^c_*/M_{\odot})<…

astro-ph.GA2022★ 3 cited

MASCOT: Molecular gas depletion times and metallicity gradients -- evidence for feedback in quenching active galaxies

C. Bertemes, D. Wylezalek, M. Albán +8

We present results from the first public data release of the MaNGA-ARO Survey of CO Targets (MASCOT), focussing our study on galaxies whose star-formation rates and stellar masses…

astro-ph.GA2022★ 33 cited

The Molecular-Gas Main Sequence and Schmidt-Kennicutt relation are fundamental, the Star-Forming Main Sequence is a (useful) byproduct

William M. Baker, Roberto Maiolino, Francesco Belfiore +8

We investigate the relationship between the star formation rate (SFR), stellar mass () and molecular gas mass () for local star-forming galaxies. We further investiga…

astro-ph.GA2022★ 63 cited

First results from the JWST Early Release Science Program Q3D: Turbulent times in the life of a extremely red quasar revealed by NIRSpec IFU

Dominika Wylezalek, Andrey Vayner, David S. N. Rupke +20

Extremely red quasars, with bolometric luminosities exceeding erg s, are a fascinating high-redshift population that is absent in the local universe. They are the…

astro-ph.GA2022

Morphology-density Relation, Quenching, and Mergers in CARLA Clusters and Proto-Clusters at

Simona Mei, Nina A. Hatch, Stefania Amodeo +11

(Abridged) To understand if the morphology-density and passive-density relations are already established at z>1.5, we study galaxies in 16 confirmed clusters at from th…

astro-ph.GA2022★ 22 cited

Probing the Inner Circumgalactic Medium and Quasar Illumination around the Reddest `Extremely Red Quasar' (ERQ)

Marie Wingyee Lau, Fred Hamann, Jarred Gillette +4

Dusty quasars might be in a young stage of galaxy evolution with prominent quasar feedback. A recently discovered population of luminous, extremely red quasars at ~2--4 has…

astro-ph.GA2022★ 12 cited

Towards a More Complete Optical Census of Active Galactic Nuclei, Via Spatially-Resolved Spectroscopy

Julia M. Comerford, James Negus, R. Scott Barrows +4

While emission-line flux ratio diagnostics are the most common technique for identifying active galactic nuclei (AGNs) in optical spectra, applying this approach to single fiber sp…

astro-ph.GA2022★ 35 cited

Ionised Gas Kinematics in MaNGA AGN. Extents of the Narrow Line and Kinematically Disturbed regions

A. Deconto-Machado, R. A. Riffel, G. S. Ilha +11

We analyse the kinematics of 170 AGN host galaxies as compared to those of a matched control sample of non-active galaxies from the MaNGA survey in order to characterise and estima…