Calibration and Correction of the Brighter-Fatter Effect in LSSTCam

DMTN-336

This living technote will be updated with descriptions of all the algorithms for Brighter-Fatter calibration and correction in the LSST DM Science Pipelines. It will include detailed descriptions of the algorithms used and deployed for specific data previews and data releases. It will also contain the verification and acceptance criteria used for calibration deployment.

Links:

• Publication URL: https://dmtn-336.lsst.io
• Alternative editions: https://dmtn-336.lsst.io/v
• GitHub repository: https://github.com/lsst-dm/dmtn-336
• Build system: https://github.com/lsst-dm/dmtn-336/actions/

Build this technical note

You can clone this repository and build the technote locally if your system has Python 3.11 or later:

git clone https://github.com/lsst-dm/dmtn-336
cd dmtn-336
make init
make html

Repeat the make html command to rebuild the technote after making changes. If you need to delete any intermediate files for a clean build, run make clean.

The built technote is located at _build/html/index.html.

Publishing changes to the web

This technote is published to https://dmtn-336.lsst.io whenever you push changes to the main branch on GitHub. When you push changes to a another branch, a preview of the technote is published to https://dmtn-336.lsst.io/v.

Editing this technical note

The main content of this technote is in index.md (a Markdown file parsed as CommonMark/MyST). Metadata and configuration is in the technote.toml file. For guidance on creating content and information about specifying metadata and configuration, see the Documenteer documentation: https://documenteer.lsst.io/technotes.