haloes going mad
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Haloes going MAD. Alexander Knebe Universidad Autonoma de Madrid. Haloes going MAD. Eyjafjallajökull brings Europe to a stand-still…. Outline. why? what? how?. Outline. why? what? how?. Why?. Millenium Simulation. Density Field. Why?. Millenium Simulation. - PowerPoint PPT PresentationTRANSCRIPT
Haloes going MAD
Haloes going MADAlexander KnebeUniversidad Autonoma de MadridHaloes going MAD
Haloes going MADEyjafjallajkull brings Europe to a stand-stillHaloes going MADOutline why?
what?
how?Haloes going MADOutline why?
what?
how?Haloes going MADWhy?
Millenium SimulationDensity FieldHaloes going MADWhy?
Millenium SimulationDensity Fieldwhere are the haloes?Haloes going MAD our beloved CDM model induces hierarchical structure formation!Why?
GHALO(a multibillion particle CDM halo)Stadel et al. (2009)Haloes going MAD our beloved CDM model induces hierarchical structure formation!Why?
GHALO(a multibillion particle CDM halo) demanding task of identifyinghaloes within haloes within haloes within haloes withinStadel et al. (2009)Haloes going MAD
halo finders...
... map simulations (reliably!) onto observables ... need to acknowledge hierarchical structuresWhy?Haloes going MAD
halo finders...
... map simulations (reliably!) onto observables ... need to acknowledge hierarchical structuresWhy?state-of-the-art cosmological simulationsrequirestate-of-the-art halo finder!thats Why!Haloes going MADOutline why?
what?
how?Haloes going MAD the dataWhat? large-scale structure simulation
zoom simulation of individual object(s)
mock haloesHaloes going MAD the dataWhat? large-scale structure simulation
MareNostrum Universe LCDM cosmology high-resolution simulation
Haloes going MAD the dataWhat? large-scale structure simulation
MareNostrum Universe LCDM cosmology high-resolution simulation
FullBox_z0.0_0256Np=2x 2563FullBox_z1.0_0256Np=2x 2563
FullBox_z0.0_0512Np=2x 5123
FullBox_z0.0_1024Np=2x 10243
Haloes going MAD
the dataWhat? large-scale structure simulation zoom simulation of individual object(s)www.clues-project.org WMAP3 cosmology high-resolution zoom
Haloes going MAD
the dataWhat? large-scale structure simulation zoom simulation of individual object(s)www.clues-project.org WMAP3 cosmology high-resolution simulation
LocalGroup_z0.0_2048
LocalGroup_z0.0_4096LocalGroup_z1.5_4096LocalGroup_z9.7_4096
[0]gas particles[1]hi-res DM particles[2]low-res DM particles[3]lower-res DM particles[4]star particles[5]lowest-res DM particles
Haloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s)www.clues-project.org WMAP3 cosmology GHALO3Stadel et al. (2009)
ghaloHaloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s)www.clues-project.org WMAP3 cosmology GHALO3Stadel et al. (2009)
ghalo-3.00400.std TIPSY format
ghaloHaloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
Haloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
ghalo
www.clues-project.org
MareNostrum UniverseHaloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
ghalo
www.clues-project.org
MareNostrum Universeenough data to poke a stick atHaloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
what what?Haloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
what what?
?Haloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
what what?
?
?Haloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
what what?
?
?and what about subhaloes?Haloes going MAD the dataWhat? large-scale structure simulation zoom simulation of individual object(s) mock haloes
what what?
?
?monday afternoon discussionHaloes going MADOutline why?
what?
how?Haloes going MAD halo finder representatives:How?Miguel Aragon CalvoDelaunay finderDaniel CeverinoBDMStefan GottloeberFOFFrancesca IannuziSUBFINDSteffen KnollmannAHFZarija LukicLANL halo finderMichal MaciejewskiHSFMark NeyrinckVOBOZSusana PlanellesASOHFDoug PotterSKIDGreg Stinsonntrpy-FOFPaul Matthew SutterpSODylan TweedAdaptaHOPMarcel Zemp6dFOFHaloes going MAD halo finder representatives:How?Miguel Aragon CalvoDelaunay finderDaniel CeverinoBDMStefan GottloeberFOFFrancesca IannuziSUBFINDSteffen KnollmannAHFZarija LukicLANL halo finderMichal MaciejewskiHSFMark NeyrinckVOBOZSusana PlanellesASOHFDoug PotterSKIDGreg Stinsonntrpy-FOFPaul Matthew SutterpSODylan TweedAdaptaHOPMarcel Zemp6dFOFmore halo finders than you could wish forHaloes going MAD halo finder representatives:How?Miguel Aragon CalvoDelaunay finderDaniel CeverinoBDMStefan GottloeberFOFFrancesca IannuziSUBFINDSteffen KnollmannAHFZarija LukicLANL halo finderMichal MaciejewskiHSFMark NeyrinckVOBOZSusana PlanellesASOHFDoug PotterSKIDGreg Stinsonntrpy-FOFPaul Matthew SutterpSODylan TweedAdaptaHOPMarcel Zemp6dFOFmore halo finders than you could wish forCODE COMPARISON PROJECT!Haloes going MAD code comparison project:How? unique definition for mass and size
mock haloes: recovering mass and size under controlled conditions
cosmological volume: mass positionstatistically! velocity
zoom simulations: haloes within haloes within haloesHaloes going MAD code comparison project:How? unique definition for mass and size
mock haloes: recovering mass and size under controlled conditions
cosmological volume: mass positionstatistically! velocity
zoom simulations: haloes within haloes within haloesHaloes going MAD code comparison project:How? unique definition for mass and size
mock haloes: recovering mass and size under controlled conditions
cosmological volume: mass positionstatistically! velocity
zoom simulations: haloes within haloes within haloesHaloes going MAD code comparison project:How? unique definition for mass and size
mock haloes: recovering mass and size under controlled conditions
cosmological volume: mass positionstatistically! velocity
zoom simulations: haloes within haloes within haloesHaloes going MAD code comparison project:How? unique definition for mass and size
mock haloes: recovering mass and size under controlled conditions
cosmological volume: mass positionstatistically! velocity
zoom simulations: haloes within haloes within haloesHaloes going MAD code comparison project:How? unique definition for mass and size
mock haloes: recovering mass and size under controlled conditions
cosmological volume: mass positionstatistically! velocity
zoom simulations: haloes within haloes within haloesfirst impressionsHaloes going MAD first impressions -- FullBoxHow?massHaloes going MADHow?position first impressions -- FullBoxusing the 10000 most massive objects onlyHaloes going MADHow?velocity first impressions -- FullBoxHaloes going MADHow?concentration first impressions -- FullBoxHaloes going MADHow?spin parameter first impressions -- FullBoxHaloes going MADHow? first impressions -- FullBoxa lot to talk aboutHaloes going MADHow?Haloes going MAD
Home Venue Rationale Program The Data Registration Practical Info
Program
Monday(codes)
09:30-10:00 welcome
10:00-11:30:
AHF (Knollmann)
ASOHF (Planelles)
pSO (Sutter)
BDM (Ceverino)
11:30-12:00 coffee
12:00-13:30:
LANL finder (Lukic)
AdaptaHOP (Tweed)
SKID (Potter)
14:00-16:00 lunch
briefing:- how were the mockhaloes generated? (Muldrew)
discussion:- how to define a halo? (chaired by Pearce)
Confirmed Halo Finder RepresentativesMiguel Aragon Calvo:Daniel Ceverino:Stefan Gottlber:Francesca Iannuzzi:Steffen Knollmann:Zarija Lukic:Michal Maciejewski:Mark Neyrinck:Susana Planelles:Doug Potter:Greg Stinson:Paul Matthew Sutter:Dylan Tweed:Marcel Zemp:
fracHOPBDMFOFSUBFINDAHFLANL halo finderHSFVOBOZASOHFSKIDntropy-FOFpSOAdaptaHOP6dFOF
Tuesday
(codes)
Wednesday
(discussions)
Thursday
(tools)Friday
(discussions)
(Mon, 24/05/2010 - Fri, 28/05/2010)
10:00-11:30
FOF (Gottloeber)
SUBFIND (Iannuzzi)
ntropy-FOF (Stinson)
HSF (Maciejewski)
11:30-12:00 coffee
12:00-13:30
6dFOF (Zemp)
VOBOZ (Neyrinck)
new (Aragon-Calvo)
14:00-16:00 lunch
10:00-11:30
- discussion of
results so far...
(chaired by Knollmann)
11:30-12:00 coffee
12:00-13:30
- addressing outstanding
questions and problems
(chaired by ? )
14:00-16:00 lunch
10:00-11:30
- merger trees
(with contributions from
Behroozi, Sinha, Coles, ...)
11:30-12:00 coffee
12:00-13:30
- how to deal with baryons?
- visualisation tools
14:00-16:00 lunch
10:00-11:30
- summary of data
analysis
- how to write a paper
out of it?
11:30-12:00 coffee
12:00
trip back to Madrid
data analysis,
comparison of results&
training sessions
data analysis,
comparison of results&
training sessions
discussion:
- what to compare? (chaired by Knebe)
Haloes going MAD