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MOONRISE: The Main MOONS GTO Extragalactic Survey
R. Maiolino, M. Cirasuolo, J. Afonso +34
The MOONS instrument possesses an exceptional combination of large multiplexing, high sensitivity, broad simultaneous spectral coverage (from optical to near-infrared bands), large…
Less than the sum of its parts: the dust-corrected H luminosity of star-forming galaxies explored at different spatial resolutions with MaNGA and MUSE
N. Vale Asari, V. Wild, A. L. de Amorim +10
The H and H emission line luminosities measured in a single integrated spectrum are affected in non-trivial ways by point-to-point variations in dust attenuation in a galaxy.…
Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C
Francesco D'Eugenio, Arjen van der Wel, Po-Feng Wu +13
We use deep, spatially resolved spectroscopy from the LEGA-C Survey to study radial variations in the stellar population of 17 spectroscopically-selected post-starburst (PSB) galax…
Comparison of stellar populations in simulated and real post-starburst galaxies in MaNGA
Yirui Zheng, Vivienne Wild, Natalia Lahén +4
Recent integral field spectroscopic (IFS) surveys have revealed radial gradients in the optical spectral indices of post-starburst galaxies, which can be used to constrain their fo…
The clustering of X-ray AGN at 0.5 < z < 4.5: host galaxies dictate dark matter halo mass
Charutha Krishnan, Omar Almaini, Nina A. Hatch +6
We present evidence that AGN do not reside in ``special'' environments, but instead show large-scale clustering determined by the properties of their host galaxies. Our study is ba…
Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
A. C. Carnall, S. Walker, R. J. McLure +19
We present a sample of 151 massive () quiescent galaxies at , based on a sophisticated Bayesian spectral energy distribution fitting analy…