TOGA

Tool for Observed Galaxy Analogs

Here you can obtain galaxy photometric catalogs drawn from cosmological hydrodynamic simulations of structure formation including a physically-motivated prescription for enriched galactic outflows. Catalogs include physical information and magnitudes.

Once you hit submit, the desired photometry will be generated, and a tar file will be created in http://ursa.as.arizona.edu/~rad/toga/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.

To select multiple options below, use the SHIFT and CONTROL keys.

Name:
Email:
Wind Models:
(select all desired)
Box sizes (Mpc/h):
(select all desired)
Redshifts:
(select all desired)
Filters-
index #s from this list
(the #s on the left),
separated by spaces:
Filters in rest
or observed frame?
Observed Frame
Rest Frame
Comments:
(optional)
Some helpful hints:

Wind Model -- Options here are described in Oppenheimer & Davé 2006. nw=no winds; cw=constant winds (see Springel & Hernquist 2003); vzw=variable momentum-driven winds.

Box size -- Simulation periodic box length in comoving Mpc/h. Note: Not all box sizes are available for all models and at all redshifts.


Please send comments or questions to Romeel Davé.