This product contains information about DESI hardware designs in machine readable formats to be used by simulations. It is intended to be correct but non-authoritative. If in question, the DocDB version of a design parameter is correct. This is intended to reflect the same information while being more conveniently organized and formatted for simulations.
PLEASE KEEP THIS FILE IN SYNC WITH THE EQUIVALENT FILE IN SVN.
The svn product described below contains only the data associated with desimodel. The code is in Github: https://github.com/desihub/desimodel.
The data that accompanies the desimodel code is not stored with the code. Due to its size, it is kept in the DESI svn repository. The public, read-only URL for svn access is https://desi.lbl.gov/svn/code/desimodel, with the usual trunk/, tags/ and branches/ directories.
Once you have installed this package, using either pip
or desiInstall
,
the associated data must also be installed. For most every case, you
should install the tag in svn that corresponds to the same tag in git.
Installing this package will create the command-line script
install_desimodel_data
. It should appear in your PATH
assuming
a successful install. install_desimodel_data --help
will show you
how to use this script.
You can also call the function desimodel.install.install()
from
inside other Python code.
When desimodel is used with other downstream code, it might become
necessary to set the environment variable DESIMODEL
.
You should set the DESIMODEL
environment variable to point to the directory
containing the data/ directory.
install_desimodel_data
with default options, may install the data in
a relatively obscure location. To find the value to set for DESIMODEL
,
you can do the following:
python -c "from importlib.resources import files; print(str(files('desimodel')))"
Files in data/inputs/ are copied from DocDB and are not intended to be used directly. These are parsed and reformatted to produce files in other data/ directories which are for use.
- data/desi.yaml
- Basic scalar parameters, organized in a nested tree.
- data/focalplane/
- Information about positioner locations and platescale.
- data/footprint/
- The areas of the sky that will be observed by DESI, with RA, Dec of tiles.
- data/sky/
- Sample sky spectra.
- data/specpsf/
- Spectrograph point-spread-function (PSF) for specter CCD pixel-level simulations.
- data/spectra/
- Example benchmark spectra.
- data/targets/
- Expected n(z) information per target class for cosmology projections.
- data/throughput/
- Throughput versus wavelength (also contained in specpsf).
- data/weather/
- Historical weather data.
There are several permanent branches that were used for testing alternative designs. Some of these will never be merged into trunk but we will keep them around for the record:
- altccd
- 500 micron versus 250 micron thick CCDs.
- bb
- Recreating assumptions used during early BigBOSS projections.
- newtiles
- An improved tiling dither pattern from Eddie Schlafly, intended to be merged prior to the start of the DESI survey.
- update_inputs
- This branch might be present during updates to the inputs to the desimodel data files. See the updating desimodel inputs document for further details.
In addition to these historical branches, there are a set of test-*
branches
that contain smaller versions of the desimodel files. These branches are
intended for use in desimodel unit tests. See the desimodel testing
document for further details.
If either the data or the code changes, a new tag should be created in both git and svn.
Please visit desimodel on Read the Docs
desimodel is free software licensed under a 3-clause BSD-style license. For details see
the LICENSE.rst
file.