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Hi Everyone,</div>
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This week our lunch talk will be given by Hua Gao, Thursday at 1pm in A113. Title and abstract are below:</div>
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<b>IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50</b></div>
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We perform a thorough analysis of the projected shapes of nearby galaxies in both observations and cosmological simulations. We implement a forward-modeling approach to overcome the limitations in previous studies, which hinder accurate comparisons between
observations and simulations. We measure axis ratios of z = 0 (snapshot 99) TNG50 galaxies from their synthetic Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) images and compare them with those obtained from real HSC-SSP images of a matched galaxy sample.
Remarkably, the comparison shows excellent agreement between the observations and the TNG50 simulation, challenging previous claims that ΛCDM models underproduced the abundance of thin galaxies. Specifically, for galaxies with stellar masses 10⩽log(M⋆/M⊙)⩽11.5,
we find ≲0.1σ tensions between the observations and the simulation, a stark contrast to the previously reported ≳10σ tensions. We reveal that low-mass galaxies (M⋆≲10^9.5M⊙) in TNG50 are thicker than their observed counterparts in HSC-SSP and attribute this
to the spurious dynamical heating effects that artificially puff up galaxies. We also find that, despite the overall broad agreement, TNG50 galaxies are more concentrated than the HSC-SSP ones at the low- and high-mass end of the stellar mass range of 9.0⩽log(M⋆/M⊙)⩽11.2
and are less concentrated at intermediate stellar masses. But we argue that the higher concentrations of the low-mass TNG50 galaxies are not likely the cause of their thicker/rounder appearances. Our study underscores the critical importance of conducting
mock observations of simulations and applying consistent measurement methodologies to facilitate proper comparison with observations.</div>
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Thanks,</div>
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Mikey</div>
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<b>Mikey Anderson Jennings</b></div>
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<b>Astronomy PhD Student </b></div>
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<b>University of Nottingham</b></div>
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<b>Centre for Astronomy and Particle Theory<br>
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