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.
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Role of gibberellins, neem leaf extract, and serine in improving wheat growth and grain yield under drought-triggered oxidative stress. [PDF]
Hameed S, Atif M, Perveen S.
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Investigating quenching in Recently Quenched Elliptical galaxies with HI studies
Recently Quenched Elliptical galaxies (RQEs) represent a critical phase in the transition from star-forming to quiescent galaxies. However, the mechanisms driving their quenching remain elusive. We conduct a multi-wavelength analysis of 155 RQEs, along with their precursors (preRQEs) and descendants (postRQEs), focusing on their neutral hydrogen (HI ...
Deo, Deepak K. +6 more
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Origins and lifetimes of secular and tidal bars in simulated disc galaxies. [PDF]
Frosst M +3 more
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The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]
Taylor ED +9 more
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Extreme properties of a compact and massive accreting black hole host in the first 500 Myr. [PDF]
Tripodi R +31 more
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Paper-Based Analytical Devices Coupled with Fluorescence Detection and Smartphone Imaging: Advances and Applications. [PDF]
Zacharis CK.
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Characterizing the luminosity components of luminous infrared galaxies in multi-wavelength from the X-ray to the far-infrared. [PDF]
Ali AAM +3 more
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A recently quenched galaxy 700 million years after the Big Bang. [PDF]
Looser TJ +44 more
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Star formation shut down by multiphase gas outflow in a galaxy at a redshift of 2.45. [PDF]
Belli S +17 more
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