News
21.07.2023:
New service: GalaxyFind
21.07.2023:
New simulation with new BH properties: Box3 (uhr)
31.05.2023:
New private simulation: LocalUniverse
25.04.2022:
Added remaining snapshots of Box4.
09.01.2023:
Added further snapshots of boxes Box2b and Box2.
23.06.2022:
Added new simulation Box4 with the stellar and ICM maps of its last snapshot.
27.05.2022:
Added ultra high-resolution stellar maps for all snapshots of Box2b and for last Box2 snapshot.
10.05.2022:
Added ultra high-resolution stellar map for Box2b, snapshot 31.
27.01.2021:
Added HaloConversion tool for computing cosmology-dependent halo masses and concentrations.
19.12.2019:
Updated to SIXTE 2.6.
07.08.2019:
Article using machine learning on mocks extracted from the Portal submitted.
18.12.2018:
First Article utilizing the Portal appeared.
10.01.2018:
Updated to SIXTE 2.0.
15.06.2017:
Instruction Movie
14.01.2017:
Chandra added. Instrument simulation for
XraySurveyor & Hitomi added.
03.07.2016:
Add SimCut service.
25.06.2016:
Add public access service.
26.04.2016:
New services: ClusterFind and ClusterInspect.
25.04.2016:
Queries to select specific merging clusters activetd
22.04.2016:
New maps in Box2: ComptonY and Shocks.
13.04.2016:
Instrument simulator is available on Phox.
11.03.2016:
AGN contribution for Phox enabled.
03.03.2016:
Phox output in SimPut format
29.02.2016:
Start test operation
PHOX
Here you can use PHOX to extract virtual X-ray observations from the Magneticum cosmological hydro simulation. See Biffi et al. 2012 and Biffi et al. 2013 for details on the code. This service is currently a prototype for Box2/hr and Box2b:hr and more simulations will be made available for virtual observation with time. This service actually executes unit_2 on our server, therefore, please log in or Register an account if you do not have one yet. See Credits how to acknowledge for this service.
SMAC
Here you can use SMAC to create your own maps of various, physical quantities for galaxy clusters from the Magneticum cosmological hydro simulation. See Dolag et al. 2005 for details of the code. It allows you to produce idealized maps of various quantities (like X-Ray, temperature, SZ, etc.) and receive a fits file image. This service is currently a prototype for Box2/hr and Box2b:hr and more simulations will be made available for map making with time. This service actually executes programs on our server, therefore, please log in or Register an account if you do not have one yet. See Credits how to acknowledge for this service.
SimCut
Here you can use SimCut to extract a Gadget (format=2) snapshot file containgn regions centered on galaxy clusters from the Magneticum cosmological hydro simulation. These shapshots will contain all original particle properties from the simulations. This service is currently a prototype for Box2/hr and Box2b:hr and more simulations will be made available for cut outs with time. This service actually executes programs on our server, therefore, please log in or Register an account if you do not have one yet. See Credits how to acknowledge for this service.
ClusterFind
Here you can use database queries to search clusters from the Magneticum cosmological hydro simulation based on their global properties. This service additionally allows you to download the data tables or to interactively produce simple scaling plots and pre-select cluster of interest to be used within the other services. See Ragagnin et al. 2017 for details of the code. Therefore, please log in or Register an account if you do not have one yet. See Credits how to acknowledge for this service.
GalaxyFind
Here you can use database queries to search satellite galaxies from the Magneticum cosmological hydro simulation based on their global properties. This service additionally allows you to download the data tables or to interactively produce simple scaling plots and pre-select galaxies of interest to be used within the other services. Please log in or Register an account if you do not have one yet. See Credits how to acknowledge for this service.
HaloConversion
The HaloConversion tool converts masses, together with the respective concentration values, between overdensities for a given set of cosmological paramters. The cosmology-dependent mass-concentration (Mc) and mass-mass (MM) relations are taken from from Magneticum hydrodynamic simulations as conversion relations presented in Ragagnin et al. (2021). See the library https://github.com/aragagnin/hydro_mc to use these relations in your own code.
