# Baryonic Physics Constraints Plan

###### tags: `parameters` `constraints`

## Overview

Goal is to construct a set of constraints that can be used to calibrate key model properties for emission lines work.

## Plan

**Bold** indicates questions that we need to figure out answers to.
*Italic* indicates possibly good places to work next.
[AJB] indicates who is working on this step.

* Mass-metallicity relation
* This already exists in the `outputAnalysisMassMetallicityBlanc2019` class in `source/output.analyses.mass_metallicity_relation.Blanc2019.F90`
* [AJB] *Add to the current constraints pipeline*
* *Estimate random and systematic error model priors?*
* Black hole mass-velocity dispersion relation
* *Find a suitable observational sample*
* Would [McConnel & Ma (2013)](https://ui.adsabs.harvard.edu/abs/2013ApJ...764..184M) sample work?
* *Implement an `outputAnalysis` class for this* (In progress...)
* Use the `outputAnalysisBlackHoleBulgeRelation` class in `source/output.analyses.black_hole_bulge_relation.F90` as an template
* New class for balck hole mass velocity dispersion implemented.
* Needs fixing
* Add to the current constraints pipeline
* Estimate random and systematic error model priors
* Star formation rate function
* Find a suitable observational sample Robotham 2011. Started creating the hdf5 file
* Implement an `outputAnalysis` class for this (Completed, PR to github)
* Use the `outputAnalysisMassFunctionStellar` class (and child classes) in `source/output.analyses.mass_function_stellar.F90` as an template

* Updated $H_{\alpha}$ luminosity function - Sobral+2013 to work with updated emission line class
* Accounts for evolution of redshift interval
* Details?
* New output analyses classes for OII luminosity function, and NII luminosity function for data from Favole+2024

IN PROGRESS
* Add to the current constraints pipeline
* Estimate random and systematic error model priors