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 |
|
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 |
For anything that requires projections,
start with x-y, x-z, y-z, and projections along the axes of the inertia tensor.