List of Key Plots
===================================

The Key Plots that demonstrate the tomographic 3x2pt power spectrum constraints
on Dark Energy are presented in Wong et al. 2025 (https://arxiv.org/abs/2501.07559)

1. Figure 6) Tomographic shear constraints on w0-wa for different numbers of equipopulated bins. Run by setting `ZBIN_TYPE=EQUI_POP`, `OBS_TYPE=1X2PT`, `FIELD=E` in the `pcl_measurement` routine.

![Shear constraints on w0-wa](https://raw.githubusercontent.com/j-hw-wong/SWEPT/refs/heads/main/docs/source/plots/contours_equipop_noise_E.png "Tomographic shear constraints")


2. Figure 8) Tomographic angular clustering constraints on w0-wa for different numbers of equipopulated bins. Run by setting `ZBIN_TYPE=EQUI_POP`, `OBS_TYPE=1X2PT`, `FIELD=N` in the `pcl_measurement` routine.

![Angular clustering constraints on w0-wa](https://raw.githubusercontent.com/j-hw-wong/SWEPT/refs/heads/main/docs/source/plots/contours_equipop_noise_N.png "Tomographic shear constraints")


3. Figure 10) Tomographic shear constraints on w0-wa for different numbers of equipopulated bins. Run by setting `ZBIN_TYPE=EQUI_POP`, `OBS_TYPE=3X2PT` in the `pcl_measurement` routine.

![3x2pt constraints on w0-wa](https://raw.githubusercontent.com/j-hw-wong/SWEPT/refs/heads/main/docs/source/plots/contours_equipop_noise_3x2pt.png "Tomographic shear constraints")