SLACR

The Simulation Lyman Alpha Comparison Repository

Here you can obtain simulated quasar spectra for a variety of ions (including Ly-alpha, CIV, and others) drawn from cosmological hydrodynamic simulations of structure formation including a physically-motivated prescription for enriched galactic outflows.

Once you hit submit, the desired spectra will be generated, and a tar file will be created in http://ursa.as.arizona.edu/~rad/slacr/your@email/your@email.tar.gz.
When ready, you will receive an email sent to your@email. You can then go to the above location and download the tar file, which contains an explanatory README file.

Please note: Your file will be deleted three days after the notification email is sent. Also, please be patient; these spectra are made hot and fresh-to-order, so they take some time! (e.g. 1000 spectra may take several hours.)

Name:
Email:
# of spectra:
Model:
Redshift:
Comments:
Some helpful hints:

# of spectra -- Each spectrum traverses the simulation volume once, parallel to the z-axis. Therefore they are short, with typical redshift interval dz<<0.1; actual dz depends on box size and redshift. Hence usually you want hundreds or even thousands of spectra. The (x,y) positions are randomly chosen. NOTE: nspectra must be a multiple of 4, or it will be reset as such.

Model -- The simulation naming convention is as follows: The number after "d" (i.e. 16,32,64) corresponds to the box size in comoving Mpc/h. The number after "n" (i.e. 256) corresponds to the number of particles: 256^3 DM and 256^3 gas particles.
Currently available model is the d-vzw15 series, described in Oppenheimer & Davé 2008. The "d" series has Omega=0.25, Lambda=0.75, H0=70, n=0.95, and Omega_b=0.044, and "vzw15" is our variable momentum-driven wind model having sigma_0=150 km/s.

Redshift -- The 16 Mpc/h box is available down to z=2, the 32 Mpc/h and 64 Mpc/h boxes down to z=0. If you request a non-existant redshift it will generate a tar file, but there will be no spectra in it and the log file will contain an error message.

Analysis -- Once you add noise and smooth to your desired spectral resolution, you may want to fit Voigt profiles with AutoVP.


Please send comments or questions to Romeel Davé.