266 citations · 2.4k across the 90 of their papers we have counts for
12 papers · 1 filter
SLOW IV: Not all that is Close will Merge in the End. Superclusters and their Lagrangian collapse regions
B. A. Seidel, K. Dolag, R. -S. Remus +4
Superclusters are the most massive structures in the universe. To what degree they are actually bound against an accelerating expansion of the background is of significant cosmolog…
PICS: Planetary Nebulae in Cosmological Simulations -- Revelations of the Planetary Nebula Luminosity Function from Realistic Stellar Populations
Lucas M. Valenzuela, Rhea-Silvia Remus, Marcelo M. Miller Bertolami +1
Even after decades of usage as an extragalactic standard candle, the universal bright end of the planetary nebula luminosity function (PNLF) still lacks a solid theoretical explana…
The MAGPI Survey: radial trends in star formation across different cosmological simulations in comparison with observations at 0.3
Marcie Mun, Emily Wisnioski, Katherine E. Harborne +20
We investigate the internal and external mechanisms that regulate and quench star formation (SF) in galaxies at using MAGPI observations and the EAGLE, Magneticum, and…
From Particles to Pixels: How many particles do I really need to construct stellar kinematic mock observational measurements?
K. E. Harborne, C. del P. Lagos, S. M. Croom +5
This work considers the impact of resolution in the construction of mock observations of simulated galaxies. In particular, when building mock integral field spectroscopic observat…
Globular cluster ages and their relation to high-redshift stellar cluster formation times from different globular cluster models
Lucas M. Valenzuela, Duncan A. Forbes, Rhea-Silvia Remus
The formation details of globular clusters (GCs) are still poorly understood due to their old ages and the lack of detailed observations of their formation. A large variety of mode…
The formation histories of massive and quiescent galaxies in the 3 < z < 4.5 Universe
Themiya Nanayakkara, Karl Glazebrook, Corentin Schreiber +16
We present the formation histories of 19 massive () quiescent (sSFR) galaxy candidates at z~3.0-4.5 observed using JWST/NIRSpec. This completes th…