Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback
Eckert D +21 more
europepmc +1 more source
A high-bias, low-variance introduction to Machine Learning for physicists. [PDF]
Mehta P +6 more
europepmc +1 more source
Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe
Pérez-González P +21 more
europepmc +1 more source
Potential applications for photoacoustic imaging using functional nanoparticles: A comprehensive overview. [PDF]
Neelamraju PM +10 more
europepmc +1 more source
openaire
Rapidly quenched galaxies in the Simba cosmological simulation and observations [PDF]
Funding: YZ acknowledges support of a China Scholarship Council - University of St Andrews Scholarship. FRM is supported by the Wolfson Harrison UK Research Council Physics Scholarship.
Yirui Zheng +2 more
exaly +2 more sources
The gas needed to sustain star formation in galaxies is supplied by the circumgalactic medium (CGM), which in turn is affected by accretion from large scales.
Shengdong Lu, Dandan Xu, Zheng Cai
exaly +2 more sources
No evidence for excess AGN activity in recently quenched massive galaxies at cosmic noon
We present an analysis of AGN activity within recently quenched massive galaxies at cosmic noon ( ∼ 2), using deep Chandra X-ray observations of the Ultra-Deep Survey (UDS) field.
Maya Skarbinski +2 more
exaly +3 more sources
The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics [PDF]
We select galaxies from the IllustrisTNG hydrodynamical simulations ( Mstars 109Mo at 0 ≤ z ≤ 2) and characterize the shapes and evolutions of their UVJ and star formation rate Cstellar mass (SFR-CMstars) diagrams.
Martina Donnari +2 more
exaly +2 more sources
The diverse star formation histories of early massive, quenched galaxies in modern galaxy formation simulations [PDF]
We present a comprehensive study of the star formation histories of massive-quenched galaxies at z = 3 in three semi-analytical models (SHARK, GAEA, GALFORM) and three cosmological hydrodynamical simulations (EAGLE, ILLUSTRISTNG, SIMBA).
Claudia del P Lagos +2 more
exaly +2 more sources

