Welcome to the repository designed for tutorials that guide you through the process of simulating and handling DESI data. A host of detailed tutorials can also be found across various DESI code repositories. However, this particular space serves primarily as a platform for:
- Tutorials that were demonstrated at specific DESI meetings, each segregated under directories marked by the date of the meeting. For example, meetings/Dec2020.
- Tutorials designed around wide-ranging subjects (like onskydata) or specific packages (such as fiberassign, redrock).
- Environment setup at NERSC
- Menu of tutorials: main DESI tutorials (primarily with a NERSC account)
- Other tutorials: legacy tutorials (some may be deprecated)
- External databases: Astro Data Lab and SPARCL: access to external databases without a NERSC account
- Acknowledgments: for DESI data licence and official acknowledgments
- For authors of tutorials
The tutorials presented here utilize a Jupyter server at NERSC. This facility enables users to access all DESI data at NERSC and work with pre-installed DESI code without necessitating any local downloads or installations.
Please note, only the tutorials located under getting_started are designed to be compatible for non-DESI NERSC users. The remainder of the tutorials demand access to DESI's private data.
To commence, you will need to create a NERSC account. DESI users can follow the instructions detailed on the DESI wiki.
Once you have a NERSC account, you can proceed to log into Perlmutter:
ssh perlmutter.nersc.gov
The role of Jupyter "kernels" is fundamental as they establish a specific set of code versions for utilization. For those who are part of the DESI collaboration, detailed guidance can be found on the collaboration wiki.
If you're not affiliated with the DESI collaboration, please refer to the instructions provided in this repository for further guidance.
To procure a copy of the tutorials on perlmutter.nersc.gov, execute:
mkdir -p $HOME/desi/git
cd $HOME/desi/git
git clone https://github.com/desihub/tutorials
Navigate to https://jupyter.nersc.gov and sign in using your credentials and OTP (One Time Password). Then, select the Perlmutter Shared CPU Node "Start" button. Using the file browser on the left, navigate to the location where you cloned the tutorials repository. ($HOME/desi/git/tutorials in the above commands). Select a tutorial to begin your journey.
If clicking on a tutorial prompts a "Select Kernel" option from a dropdown list, it indicates that the default tutorial kernel on GitHub is not among the kernels already installed on your system. The system is thus asking you to choose from the kernels you do have installed. While most tutorials are compatible with the latest release (for instance, 23.1), some tutorials may require a specific release, which will be indicated at the top of the tutorial. If this is the case, return to perlmutter.nersc.gov, run
source $CFS/desi/software/desi_environment.sh main
$DESIMODULES/install_jupyter_kernel.sh VERSION
for the necessary VERSION, and refresh the Jupyter page.
This repository hosts a selection of tutorials, including:
-
Getting started (
getting_started) These tutorials are centered around the public data releases:- EDR_AnalyzeZcat.ipynb: This tutorial guides you through the process of flagging a unique set of primary (that is, optimal) spectra for a particular object in the EDR catalog and applying fundamental quality cuts. It showcases how to disaggregate the data in the combined catalog based on target type (BGS, LRG, etc.), survey (SV1, SV2, etc.), and the quantity of spectra per target. Additionally, it demonstrates how to extract and depict various spectra of the same target.
- intro_to_DESI_EDR_files.ipynb: This tutorial offers an exploration into the DESI data file structure in the Early Data Release (EDR). It instructs you on how to access different files in the data release, retrieve all available spectra along with redshift information for a specific object, and eventually plot the "best" spectrum.
- figures_from_EDR_paper.md: Links to the relevant files to replicate the primary figures featured in the Early Data Release paper
-
DESI meetings (
meetings)-
DESI Meeting Dec 2020
- Dec2020/LSS.ipynb
- Dec2020/ML_TensorFlow/ML_TensorFlow.ipynb
- Dec2020/galaxies/fitting_redshifts.ipynb
- Dec2020/galaxies/fitting_sps.ipynb
- Dec2020/quickquasars/quickquasars.ipynb
-
DESI Meeting June 2021
- June2021/Intro_to_a_DESI_Release.ipynb
- June2021/git-intro.ipynb
- June2021/nersc_computing/computing_at_nersc.ipynb
-
DESI Meeting Dec 2021
- Dec2021/Everest_Tutorial_Dec2021.ipynb
- Dec2021/SpectroperfectionismExample.ipynb
-
-
Fiber assignment (
fiberassign)- FiberAssign.ipynb: fiber assignment basics
- FiberAssignDECaLS.ipynb: use observational data from DR8 to prepare it for fiberassign
- FiberAssignMocks.ipynb: Generate mock files from simulations to feed into fiberassign
- FiberAssignAlgorithms_Part1.ipynb: a detailed look at fiberassign algorithms
- FiberAssignAlgorithms_Part2.ipynb: fiberassign with multiple survey passes
- fiberassign/restrict_reach.ipynb
-
Redrock (
redrock)- RedrockBOSSDemo.ipynb
- RedrockNthBestFit.ipynb: How to look up the Nth best redrock fit coefficients.
- RedrockOutputs.ipynb: Understanding redrock outputs and connecting the coefficients to template spectra.
- redshift-database.ipynb : interacting with DESI pipeline and redshift data in a database (work in progress).
-
On sky data (
onskydata):- spectro_completeness.ipynb: computing spectroscopic completeness on DESI data.
- spectro_nz.ipynb: making an n(z) histogram from the spectro production zbest files.
- Intro_to_DESI_SV_spectra.ipynb: working with real DESI data from minisv2
- EDR_Tutorial.ipynb: tutorial notebook to work with EDR data.
- Spectroscopic Production Database tutorial: working with EDR data in a database.
-
archive
- archive/GFA_targets.ipynb
- archive/Intro_to_DESI_spectra.ipynb
- archive/dc17a-truth.ipynb
- archive/quickgen.ipynb
- archive/simulating-desi-spectra.ipynb: how to simulate your own spectra
- archive/survey-simulations.ipynb: how to use "survey simulation" outputs
These links allow you to browse the results of these tutorials from GitHub; to run them yourself follow the instructions in the "Getting started" section above.
Tutorials hosted in other packages include (but haven't been recently vetted):
- How to run survey simulations.
- How to convert an SED into a simulated DESI spectrum
- How to run fiber assignment
- How to run quicksurvey catalog-level simulations
- How to make all-sky plots
- Working with DESI target bits (Main, CMX, SV)
In addition to the database access through NERSC, one can use the following external database services.
The Astro Data Lab serves a copy of the DESI EDR database as desi_edr. This is accessible to users without a NERSC account.
Various modes of data access are described here.
In particular, there is a Table Access Protocol (TAP) handle that provides a convenient access layer for the
DESI catalog database tables. TAP-aware clients (such as TOPCAT) can point to https://datalab.noirlab.edu/tap,
select the desi_edr database, and see the database tables and descriptions.
Descriptions of the associated tables can also be found in the Data Lab table browser and on the DESI Data Documentation Database page.
The SPectra Analysis & Retrievable Catalog Lab (SPARCL) contains DESI EDR spectra that were coadded per healpix. It is a searchable database that can be used via the Astro Data Lab JupyterLab Notebook. Alternatively, the Python client can be installed locally using:
pip install sparclclient
The client can be loaded within a Python session or program via:
>>> from sparcl.client import SparclClient
>>> client = SparclClient()
There are instructions and useful examples in the How-to-use-SPARCL tutorial notebook.
Any use of DESI data whether via NERSC or external databases requires DESI Data Acknowledgments.
Include at the beginning of the tutorial what is needed as a prerequisite for running the tutorial, e.g. specific codes, environment variables, datasets. It's OK to link elsewhere for detailed instructions (e.g. for how to install DESI code in general).