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The Quenching of Cluster Galaxies
In this thesis we present two projects investigating the evolution and quenching of cluster galaxy star formation (SF) activity. Leveraging a sample of 36 galaxy clusters, we measure the level of member SF activity. Over the 7.5 billion years spanned by our clusters, from z=1.5 to z=0.15, the SF activity of cluster galaxies decreases by a factor of 11.openaire +1 more source
Galaxies at redshifts 5 to 6 with systematically low dust content and high [C ii] emission
Nature, 2015Caitlin Casey +2 more
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A new population of recently quenched elliptical galaxies in the SDSS
Monthly Notices of the Royal Astronomical Society, 2014Eric F Bell, Anna Gallazzi, Tim Haines
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SDSS-IV MaNGA: evidence of the importance of AGN feedback in low-mass galaxies
Monthly Notices of the Royal Astronomical Society, 2018Samantha J Penny +2 more
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Properties of galaxies reproduced by a hydrodynamic simulation
Nature, 2014Debora Šijački +2 more
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High molecular gas fractions in normal massive star-forming galaxies in the young Universe
Nature, 2010Linda Tacconi +2 more
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Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6
Nature, 2017Eduardo Banados +2 more
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STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
Annual Review of Astronomy and Astrophysics, 1998Robert C Kennicutt
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