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Chronos and KAIROS: MOSFIRE observations of post-starburst galaxies in z ∼ 1 clusters and groups [PDF]
We present an exploration of ∼500 spectroscopically confirmed galaxies in and around two large-scale structures (LSSs) at z ∼ 1 drawn from the Observations of Redshift Evolution in Large Scale Environments survey, an ongoing, wide-field photometric and ...
Brian Lemaux, L M Lubin, G K Squires
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Post-starburst galaxies in simulations and observations
2022Post-starburst (PSB) galaxies are the galaxies in which star formation has recently been sharply truncated, as indicated by strong Balmer absorption lines alongside weak or absent nebular emission lines. PSBs are believed to be an important transitional state between the star- forming and quiescent populations, and could be important candidates for the
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The UV enigma of post-starburst galaxies
Astrophysics and Space Science, 2014We have studied the panchromatic broad-band properties from the FUV to the MIR of a sample of 808 post-starburst galaxies. We find that in the optical and near-IR bands post-starburst galaxies (PSGs) form a remarkably uniform class of objects and that, on average, simple populations synthesis models (SSP) reproduce very well the SEDs of PSGs over a ...
Melnick, J, De Propris, R
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The evolution of post-starburst galaxies from z=2 to 0.5 [PDF]
V. W. and K. R. acknowledge support of the European Research Council via the award of a starting grant (SEDMorph; P.I. V. Wild).We present the evolution in the number density and stellar mass functions of photometrically selected post-starburst galaxies ...
Kate Rowlands +2 more
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Rise and fall of post-starburst galaxies in Magneticum Pathfinder
Monthly Notices of the Royal Astronomical Society, 2021Andreas Burkert +2 more
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Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
Monthly Notices of the Royal Astronomical Society, 2020Rachel Bezanson +2 more
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The origins of post-starburst galaxies at z < 0.05
Monthly Notices of the Royal Astronomical Society, 2018Yirui Zheng +2 more
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