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tests:discs:mockub [2014/11/03 09:35] kawatatests:discs:mockub [2022/10/24 12:26] (current) – external edit 127.0.0.1
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 ====== Barcelona Mock data Suite ====== ====== Barcelona Mock data Suite ======
- 
-Readme file for the Barcelona mock data: 12 columns:  
-first 6 columns: (x,y,z,vx,vy,vz) without errors, 
-last 6 columns: (x,y,z,vx,vy,vz) with errors. Galactocentric coordinates, positions in kpc and velocities in km/s. 
- 
-Barcelona test particle simulation RC sample with bar potential (old error model) {{:tests:discs:outmr_3_short.dat|}} 
- 
-Barcelona Nbody simulation RC sample with Bar potential (new error model) {{:tests:discs:simb5.gc.dat|}} 
- 
-Barcelona test particle simulation A0 sample with density wave spiral arms (new error model) {{:tests:discs:simtwa.gc.dat|}} 
  
  
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 **The simulation data is too large to upload it to the twiki. We can provide it in a USB stick or you can find it at google drive: https://docs.google.com/file/d/0B8sgZGL4aKpSc3dlUnRKdkszaHM/edit?usp=sharing .** **The simulation data is too large to upload it to the twiki. We can provide it in a USB stick or you can find it at google drive: https://docs.google.com/file/d/0B8sgZGL4aKpSc3dlUnRKdkszaHM/edit?usp=sharing .**
  
 +===== N-body data =====
 +
 +===Pure N-body, isolated galaxy (barred)===
 +
 +-You can find a snapshot of this model (B1), that has 1 million disk particles, at: 
 +
 +Barcelona Nbody simulation 1M particles, barred model + spirals connected to the bar, centered at the Galactic Centre and bar pattern speed of 37-38 km/s/kpc. {{:tests:discs:isol_b1_stars_centered.dat.gz|}}
 +
 +http://www.am.ub.edu/~sroca/Nbody/snapshots/B1/isol_B1_stars_x8.5kpc.out (the center is at a solar position, the sun is placed in the x axis at 8.5 kpc from the galactic center)
 +
 +-In each row you will find: 
 +
 +x(kpc),y(kpc),z(kpc),vx(km/s),vy(km/s),vz(km/s),mass (Msun)
 +
 +
 +-If the user needs more snapshots from this simulation please do not hesitate to contact with Santi Roca-Fabrega (sroca@am.ub.es).
 +
 +-If using this simulation for a publication please use the following references: Roca-Fabrega et al 2013 (2013MNRAS.432.2878R) and Roca-Fabrega et al. 2014 (2014MNRAS.440.1950R)
 +
 +
 +
 +--Pure N-body, isolated galaxy (unbarred)--
 +
 +-You can find a snapshot of this model (U1), that has 1 million disk particles, at: 
 +
 +http://www.am.ub.edu/~sroca/Nbody/snapshots/U1/isol_U1_stars_centered.out (centered to the galactic center)
 +http://www.am.ub.edu/~sroca/Nbody/snapshots/U1/isol_U1_stars_x8.5kpc.out (the center is at a solar position, the sun is placed in the x axis at 8.5 kpc from the galactic center)
 +
 +-In each row you will find: 
 +
 +x(kpc),y(kpc),z(kpc),vx(km/s),vy(km/s),vz(km/s),mass (Msun)
 +
 +
 +-If the user needs more snapshots from this simulation please do not hesitate to contact with Santi Roca-Fabrega (sroca@am.ub.es).
 +
 +-If using this simulation for a publication please use the following references: Roca-Fabrega et al 2013 (2013MNRAS.432.2878R) and Roca-Fabrega et al. 2014 (2014MNRAS.440.1950R)
 +Model B1 (barred model + spirals connected to the bar, 1*10^6 disk particles)
 +
 +
 +Barcelona Nbody simulation RC sample with Bar potential (with extinction, new error model) {{:tests:discs:simb5.gc.dat|}}
 +
 +===Cosmological N-body + hydrodynamics===
 +
 +-You can find a snapshot of the stellar component that is inside 500kpc from the center of the main galactic 
 +system in this simulation, at redshift 0, in: 
 +
 +http://www.am.ub.edu/~sroca/Hidrosim/MW_003/RUN2.3/all_stars_z0.0_r500kpc_centered.out (centered to the galactic center)
 +http://www.am.ub.edu/~sroca/Hidrosim/MW_003/RUN2.3/all_stars_z0.0_r500kpc_x8.5kpc.out (the center is at a solar position, the sun is placed in the x axis at 8.5 kpc from the galactic center)
 +
 +-In each column you can find:
 +
 +x(kpc),y(kpc),z(kpc),vx(km/s),vy(km/s),vz(km/s),mass (Msun), iron (solar), alpha/iron (solar), age(Gyrs), redshift_birth , param1, param2, vcirc (km/s, GM/r approach)
  
 +-If the user needs more snapshots from this simulation please do not hesitate to contact with Santi Roca-Fabrega (sroca@am.ub.es).
  
 +-If using this simulation for a publication please use the following references: Roca-Fabrega et al 2015 (2015arXiv150406261R)
tests/discs/mockub.1415007324.txt.gz · Last modified: 2022/10/24 12:26 (external edit)