Workshop Projects
project |
lead |
participants |
comments |
full physics paper |
Federico Sembolini |
everyone |
paper II in the comparison series presenting the full physics runs (last version: 22 Feb 2016)
|
effects of baryons |
Weiguang Cui |
Federico Sembolini, Gustavo Yepes
|
Paper (draft) uploaded to paper.pdf (updated version 15 Dec. 2015)
|
substructure |
Pascal Elahi |
|
Paper on subhaloes/galaxies in nIFTy Cluster 00019 almost finished
|
black holes |
Stuart Muldrew/Rob Thacker |
Qin Fei
|
|
weak gravitational lensing |
Madhura Killedar |
Hareth Mahdi, Pascal Elahi, Jesus Vega |
|
strong gravitational lensing |
Hareth Mahdi
|
Pascal Elahi, Madhura Killedar, Jesus Vega
|
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galaxy dynamics |
Lyndsay Old |
Matt Owers, Katherine Harborne, George Woodhouse
|
|
ICL |
Weiguang Cui |
Chris Lidman, Sara Brough, Madhura Killedar, Dan Taranu |
start with simulated images... |
X-rays |
Matt Owers |
Weiguang Cui, Elena Rasia, Veronica Biffi |
start with simulated images... |
SZ |
Federico Sembolini |
Gustavo Yepes |
start with simulated images... |
BCG @ z=0 |
Sara Brough |
|
|
BCG evolution |
Stuart Muldrew |
|
|
BCG: SAMs vs FP |
Daniel Cunnama |
Pascal Elahi |
|
Orbits: environment |
Matt Owers |
Pascal Elahi |
|
Orbits: phase-space |
Lyndsay Old |
|
|
Orbits: pre-processing |
Pierluigi Cerulo |
Frazer Pearce |
|
Orbits: transformations |
Daniel Cunnama |
Simon Deeley, Michael Drinkwater |
|
Baryon Distribution in
cluster outskirts.
|
Chris Power
|
|
How is gas coming into the cluster? What is the temperature structure and likely magnetic field structure? How detectable is this likely to be?
|
Substructure in wider region |
Jake Arthur |
Frazer Pearce, Pascal Elahi, Meghan Gray, Alex Knebe |
Repeat analysis from substructure paper out to 6Mpc. Contrast galaxies not in cluster with those in the cluster
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For anything that requires projections,
start with x-y, x-z, y-z, and projections along the axes of the inertia tensor.
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