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Extreme Horizon

Extreme Horizon

Resolving galactic disks in their cosmic environment

Orion

Orion

Molecular cloud fragmentation and evolution, formation of prestellar cores

Fragdisk

Fragdisk

Fragmentation of self-gravitating disks

Synthetic disk populations

Synthetic disk populations

Resolving protoplanetary disks in massive protostellar clumps

Wind of HD189733

Wind of HD189733

Unveiling the magnetic link between stars and planets

Dusty collapses

Dusty collapses

Understanding the dynamics of dust during the protostellar collapse

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  1. Home
  2. Cosmology
  3. Extreme Horizon
  4. Extreme Horizon (50 Mpc run)
  5. $Z \sim 2$
  6. Galaxy catalog

Acknowledgement

Project acknowledgement

To acknowledge this project, please cite :

               @ARTICLE{2020A&A...643L...8C,
                   author = {{Chabanier}, S. and {Bournaud}, F. and {Dubois}, Y. and {Codis}, S. and {Chapon}, D. and {Elbaz}, D. and {Pichon}, C. and {Bressand}, O. and {Devriendt}, J. and {Gavazzi}, R. and {Kraljic}, K. and {Kimm}, T. and {Laigle}, C. and {Lekien}, J. -B. and {Martin}, G. and {Palanque-Delabrouille}, N. and {Peirani}, S. and {Piserchia}, P. -F. and {Slyz}, A. and {Trebitsch}, M. and {Y{\`e}che}, C.},
                   title = "{Formation of compact galaxies in the Extreme-Horizon simulation}",
                   journal = {\aap},
                   keywords = {galaxies: formation, galaxies: evolution, galaxies: high-redshift, galaxies: structure, methods: numerical, Astrophysics - Astrophysics of Galaxies},
                   year = 2020,
                   month = nov,
                   volume = {643},
                   eid = {L8},
                   pages = {L8},
                   doi = {10.1051/0004-6361/202038614},
                   archivePrefix = {arXiv},
                   eprint = {2007.04624},
                   primaryClass = {astro-ph.GA},
                   adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...643L...8C},
                   adsnote = {Provided by the SAO/NASA Astrophysics Data System}
               }

Galactica database acknowledgement

If you use it in your own work, you may acknowledge the origin of the data obtained on the Galactica database like so:

This work reused datasets available on the Galactica simulations database
(http://www.galactica-simulations.eu)
                            
Cite me
Frédéric BOURNAUD  

Galaxy catalog

Galaxy catalog (37698 galaxy objects)

We detected galaxies with more than 50 stellar particles (about $10^{8} \; \Msun$) using AdaptaHOP (Aubert et al. 2004). There are 37 698 galaxies detected in Extreme Horizon at $z\sim2$ and 20 314 in Standard Horizon. While the mass functions above $10^{10} \; \Msun$ are quite similar in both simulations, Extreme Horizon forms twice as many galaxies as Standard Horison with stellar mass $\textrm{M}_{*} \le 5\times 10^{9} \; \Msun$. We rule out any detection bias since stellar particles have similar masses in both simulations (new stars form at the maximal resolution level in each simulation) and we attribute this difference to the increased resolution in low-density regions.

Here is an interactive (rotating/zoomable) 3D scatterplot of the full galaxy catalog with point sizes scaling with the galaxy total mass and point colors scaling with the stellar mass :

Datafiles
Catalog 3D scatterplot data
This is a 3D scatterplot JSON file for interactive rendering of the galaxy 3D coordinates in the simulation box
  • JSON 
Search filters

Set custom search filters to get your own galaxy subset.

Field Unit Range Min. Mean Max. Std dev.
$\textrm{Mpc} \cdot \textrm{h}^{-1}$
0.002 25.734 49.999 13.738
$\textrm{Mpc} \cdot \textrm{h}^{-1}$
0.005 26.303 49.999 14.298
$\textrm{Mpc} \cdot \textrm{h}^{-1}$
0.001 25.386 50.000 15.106
$\textrm{kpc} \cdot \textrm{h}^{-1}$
0.000 0.178 2.979 0.091
$\textrm{kpc} \cdot \textrm{h}^{-1}$
0 0.087 1.084 0.032
$\textrm{M}_{\odot}$
1412999936 21235593216 3179000102912 72646967296
$\textrm{M}_{\odot}$
0 1493141248 277211676672 5604392960
0 0.000 1 0.016
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This material is Open Data