.. image:: https://readthedocs.org/projects/nemo-sz/badge/?version=latest
Nemo is a millimeter-wave Sunyaev-Zel'dovich galaxy cluster and
compact source detection package, originally developed for the
Atacama Cosmology Telescope <https://act.princeton.edu/>
project,
and capable of analyzing maps that will be produced by the
Simons Observatory <https://simonsobservatory.org/>
.
BSD 3-Clause <https://github.com/simonsobs/nemo/blob/main/LICENSE>
_pip install nemo-sz
GitHub issues page <https://github.com/simonsobs/nemo/issues>
,
and/or contact Matt Hilton <mailto:matt.hilton@mykolab.com>
.Nemo is written in Python <https://www.python.org/>
and
provides several modules <https://nemo-sz.readthedocs.io/en/latest/reference.html>
that
may be useful for analyzing ACT/SO data, in addition to the command-line programs provided
in the package.
Nemo is not the pipeline used for
Hasselfield et al. (2013) <http://adsabs.harvard.edu/abs/2013JCAP...07..008H>
, but implements many
of the ideas presented there. It is the package that was used to produce the
ACT DR3 cluster catalog <https://ui.adsabs.harvard.edu/abs/2018ApJS..235...20H/abstract>
,
and the ACT DR5 cluster catalog <https://ui.adsabs.harvard.edu/abs/2020arXiv200911043H/abstract>
_.
All ACT data products are available from LAMBDA <https://lambda.gsfc.nasa.gov/product/act/actpol_prod_table.cfm>
_.
Nemo is under active development, and not all documentation or example config files are up to date (some may contain references to files that are not yet publicly available). The package also contains some experimental features that are not necessarily well tested.
If you need to acknowledge the use of Nemo, please cite
Hilton et al. (2021) <https://ui.adsabs.harvard.edu/abs/2020arXiv200911043H/abstract>
_.