Published September 8, 2025 | Version v1
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Supplementary material of CTAO publication "Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory "

  • 1. University of Padova, Department of Physics and Astronomy
  • 2. ROR icon National Institute for Astrophysics
  • 3. ROR icon University of Rome Tor Vergata

Description

This repository allows to reproduce almost the complete analysis and the plots of the publication "Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory " of the CTAO, currently submitted for publication in MNRAS, and available in preprint https://arxiv.org/abs/2508.19120. It contains also additional material that is not reported in the publication such as tables of astrophysical factors, that could be used separately.

Breakdown of the content:

1/ Clumpy DM density and astrophysical profiles

Clumpy is the open source public software used for the generation of DM density profiles and astrophysical factors for the work. In the `clumpy` folder one can find

1A/ Clumpy density profiles, that contains the density profiles in function of the angular distance from the dsph center (as well as a README to explain its content):

clumpy/DMdensity/
clumpy/DMdensity/README.md
clumpy/DMdensity/dm_densityprofile_burkert.dat
clumpy/DMdensity/dm_densityprofile_burkert_others.dat
clumpy/DMdensity/dm_densityprofile_einasto.dat
clumpy/DMdensity/dm_densityprofile_einasto_others.dat

1B/ Clumpy annihilating-DM astrophysical profiles for Einasto and Burkert profiles, that contains the median and +-1/2 sigma profiles in function of the angular distance, in the clumpy format:

clumpy/Jfactors/profile/Burkert/README.md
clumpy/Jfactors/profile/Burkert/rvir_BooI_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_CBe_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_DraI_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_GruII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_RetII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_Scl_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_Seg1_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_Sex_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_SgrII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_SgrI_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_TriII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_UMaII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_UMi_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Burkert/rvir_Wil1_MCMC.dat.Jalphaint_cls.output

clumpy/Jfactors/profile/Einasto/rvir_BooI_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_CBe_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_DraI_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_GruII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_RetII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_Scl_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_Seg1_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_Sex_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_SgrII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_SgrI_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_TriII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_UMaII_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_UMi_MCMC.dat.Jalphaint_cls.output
clumpy/Jfactors/profile/Einasto/rvir_Wil1_MCMC.dat.Jalphaint_cls.output

1C/ the same but for the decay-astrophysical factors. 

clumpy/Dfactors/profile/Burkert/rvir_BooI_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_CBe_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_DraI_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_GruII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_RetII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_Scl_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_Seg1_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_Sex_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_SgrII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_SgrI_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_TriII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_UMaII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_UMi_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Burkert/rvir_Wil1_MCMC.dat.Dalphaint_cls.output

clumpy/Dfactors/profile/Einasto/rvir_BooI_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_CBe_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_DraI_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_GruII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_RetII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_Scl_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_Seg1_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_Sex_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_SgrII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_SgrI_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_TriII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_UMaII_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_UMi_MCMC.dat.Dalphaint_cls.output
clumpy/Dfactors/profile/Einasto/rvir_Wil1_MCMC.dat.Dalphaint_cls.output

1D/ The corresponding 2Dmaps (fits file) generated with `gammapy`:

clumpy/Dfactors/2Dmaps/Burkert/decay_CBe2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Burkert/decay_DraI2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Burkert/decay_RetII2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Burkert/decay_Scl2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Burkert/decay_SgrII2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Burkert/decay_UMaII2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Burkert/decay_UMi2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Burkert/decay_Wil12D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits

clumpy/Dfactors/2Dmaps/Einasto/decay_CBe2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Einasto/decay_DraI2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Einasto/decay_RetII2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Einasto/decay_Scl2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Einasto/decay_SgrII2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Einasto/decay_UMaII2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Einasto/decay_UMi2D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits
clumpy/Dfactors/2Dmaps/Einasto/decay_Wil12D_FOVdiameter10.0deg_nside1024-DFACTOR-Dtot-image.fits

along with the script to generate them:

clumpy/Jfactors/2Dmaps/makeFitsImage.py

clumpy/Dfactors/2Dmaps/makeFitsImage.py

2/ The instrument response functions of CTAO (Prod5.1)

The analysis is based on Prod5.1 CTAO IRFs available at https://doi.org/10.5281/zenodo.5499840. The folder

IRFs/HOWTO.md

contains an instruction file to retrieve the IRFs and place them correctly to run scripts.

3/ The actual limits (sigmav, tau) obtained from our analysis, expressed in quantiles.

These comes 

  • from single targets or combined targets,
  • for annihilation and decay,
  • for Burkert or Einasto profiles
  • considering the astrophysical factor as a nuisance parameter (`wsj`) or not (`wosj`)

3.1/ Annihilation sigmav limits without J-factor as nuisance

limits_wosj/annihilation/combined/Combined_annichilation_CBe_Wil1_t600_wosj_quantiles.csv
limits_wosj/annihilation/combined/Combined_annihilation_AllSources_t600_wosj_quantiles.csv

limits_wosj/annihilation/single/CBe_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/CBe_einasto_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/DraI_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/DraI_einasto_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/RetII_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/RetII_einasto_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/Scl_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/Scl_einasto_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/SgrII_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/SgrII_einasto_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/UMaII_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/UMaII_einasto_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/UMi_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/UMi_einasto_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/Wil1_burkert_annihilation_t100h_wosj_quantiles.csv
limits_wosj/annihilation/single/Wil1_einasto_annihilation_t100h_wosj_quantiles.csv

3.2/ Decay lifetime limits without J-factor as nuisance

limits_wosj/decay/combined/Combined_decay_einasto_AllSources_t600_wosj_quantiles.csv
limits_wosj/decay/combined/Combined_decay_einasto_CBe_UMi_t600_wosj_quantiles.csv

limits_wosj/decay/single/CBe_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/CBe_einasto_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/DraI_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/DraI_einasto_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/RetII_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/RetII_einasto_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/Scl_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/Scl_einasto_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/SgrII_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/SgrII_einasto_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/UMaII_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/UMaII_einasto_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/UMi_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/UMi_einasto_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/Wil1_burkert_decay_t100h_wosj_quantiles.csv
limits_wosj/decay/single/Wil1_einasto_decay_t100h_wosj_quantiles.csv

3.3/ Annihilation cross-section limits with J-factor as nuisance

limits_wsj/annihilation/combined/combined_burkert_annihilation_DraI_UMi_t600_wsj_quantiles.csv
limits_wsj/annihilation/combined/combined_burkert_annihilation_allSources_t600_wsj_quantiles.csv
limits_wsj/annihilation/combined/combined_einasto_annihilation_CBe_Wil1_t600_wsj_quantiles.csv
limits_wsj/annihilation/combined/combined_einasto_annihilation_DraI_UMi_t600_wsj_quantiles.csv
limits_wsj/annihilation/combined/combined_einasto_annihilation_allSources_t600_wsj_quantiles.csv

limits_wsj/annihilation/single/CBe_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/CBe_einasto_annihilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/DraI_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/DraI_einasto_annihilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/RetII_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/RetII_einasto_annihilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/Scl_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/Scl_einasto_annihilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/SgrII_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/SgrII_einasto_annihilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/UMaII_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/UMaII_einasto_annihilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/UMi_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/UMi_einasto_annihilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/Wil1_burkert_annichilation_t100_wsj_quantiles.csv
limits_wsj/annihilation/single/Wil1_einasto_annihilation_t100_wsj_quantiles.csv

3.4/ Decay lifetime limits with J-factor as nuisance

limits_wsj/decay/combined/combined_burkert_decay_DraI_UMi_t600_wsj_quantiles.csv
limits_wsj/decay/combined/combined_burkert_decay_allSources_t600_wsj_quantiles.csv
limits_wsj/decay/combined/combined_einasto_decay_CBe_Wil1_t600_wsj_quantiles.csv
limits_wsj/decay/combined/combined_einasto_decay_DraI_UMi_t600_wsj_quantiles.csv
limits_wsj/decay/combined/combined_einasto_decay_allSources_t600_wsj_quantiles.csv

limits_wsj/decay/single/CBe_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/CBe_einasto_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/DraI_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/DraI_einasto_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/RetII_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/RetII_einasto_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/Scl_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/Scl_einasto_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/SgrII_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/SgrII_einasto_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/UMaII_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/UMaII_einasto_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/UMi_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/UMi_einasto_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/Wil1_burkert_decay_t100_wsj_quantiles.csv
limits_wsj/decay/single/Wil1_einasto_decay_t100_wsj_quantiles.csv

4/ Plotting parts

These notebooks were used to plot figures. When the paper will be accepted, we will add figure numbers.

4.1/ DM profiles and astrophysical profiles

plots/plots_dm_profiles/makeplot_dm_2dmap_profiles.ipynb
plots/plots_dm_profiles/makeplot_dm_astro_profiles_14.ipynb
plots/plots_dm_profiles/makeplot_dm_density_profile_14.ipynb
plots/plots_dm_profiles/makeplot_dmspectra.ipynb

 

plots/ctao_ksp_dsphs.yaml

plots/plots_dm_profiles/2Dmaps_dsph_parameters.csv
plots/plots_dm_profiles/AstroProfiles_dsph_parameters_14.csv
plots/plots_dm_profiles/Density_dsph_parameters_14.csv

4.2/ DM profiles and astrophysical profiles

plots/plots_limits/makeplot_dsphKSP_ann_dec.ipynb
plots/plots_limits/makeplot_limits_combined_ann_bb.ipynb
plots/plots_limits/makeplot_limits_combined_ann_dec_allch.ipynb
plots/plots_limits/makeplot_limits_combined_dec_bb.ipynb
plots/plots_limits/makeplot_limits_single_ann.ipynb
plots/plots_limits/makeplot_limits_single_decay.ipynb

with additional input files

plots/plots_limits/Relic_WIMP_Abundance.tsv

plots/plots_limits/dmbounds/ando_2015_fig4_decay_bb.ecsv
plots/plots_limits/dmbounds/cirelli_2012_cta_fornax_decay_bb.csv
plots/plots_limits/dmbounds/cirelli_2012_cta_fornax_decay_tautau.csv
plots/plots_limits/dmbounds/collider_2015_atlascms_ann_bb.ecsv
plots/plots_limits/dmbounds/collider_2015_atlascms_ann_tautau.ecsv
plots/plots_limits/dmbounds/cta_2021_gc_WW_core.ecsv
plots/plots_limits/dmbounds/cta_2021_gc_ann_bb_sens.ecsv
plots/plots_limits/dmbounds/cta_2021_gc_ann_tautau_sens.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_WW_sens_ISOmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_WW_sens_ISOmean.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_WW_sens_NFWmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_WW_sens_NFWmean.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_bb_sens_ISOmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_bb_sens_ISOmean.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_bb_sens_NFWmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_bb_sens_NFWmean.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_mumu_sens_ISOmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_mumu_sens_ISOmean.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_mumu_sens_NFWmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_mumu_sens_NFWmean.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_tautau_sens_ISOmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_tautau_sens_ISOmean.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_tautau_sens_NFWmax.ecsv
plots/plots_limits/dmbounds/cta_2023_LMC_ann_tautau_sens_NFWmean.ecsv
plots/plots_limits/dmbounds/cta_2023_perseuscluster_dec_bb_sens.ecsv
plots/plots_limits/dmbounds/cta_2023_perseuscluster_dec_tautau_sens.ecsv
plots/plots_limits/dmbounds/cta_perseus_ksp_bb.csv
plots/plots_limits/dmbounds/cta_perseus_ksp_tautau.csv
plots/plots_limits/dmbounds/cta_subhalo_bb.ecsv
plots/plots_limits/dmbounds/cta_subhalo_tautau.ecsv
plots/plots_limits/dmbounds/directsearches_2015_coupp_ann_bb.ecsv
plots/plots_limits/dmbounds/directsearches_2015_coupp_ann_tautau.ecsv
plots/plots_limits/dmbounds/hawc_2018_multidsph_ann_bb_notri2.ecsv
plots/plots_limits/dmbounds/hawc_2018_multidsph_ann_tautau_notri2.ecsv
plots/plots_limits/dmbounds/hess_2020_multidsph_ann_bb.ecsv
plots/plots_limits/dmbounds/hess_2020_multidsph_ann_tautau.ecsv
plots/plots_limits/dmbounds/lat_2012_gc_dec_bb.ecsv
plots/plots_limits/dmbounds/lat_2016_multidsph_dec_bb.ecsv
plots/plots_limits/dmbounds/lat_2016_multidsph_dec_tautau.ecsv
plots/plots_limits/dmbounds/lat_2023_multidsph_ann_bb_measured.ecsv
plots/plots_limits/dmbounds/lat_2023_multidsph_ann_tautau_measured.ecsv
plots/plots_limits/dmbounds/lhaaso_2024_multidsph_ann_bb.ecsv
plots/plots_limits/dmbounds/lhaaso_2024_multidsph_ann_tautau.ecsv
plots/plots_limits/dmbounds/lhaaso_2024_multidsph_dec_bb.ecsv
plots/plots_limits/dmbounds/lhaaso_2024_multidsph_dec_tautau.ecsv
plots/plots_limits/dmbounds/magic_2018_perseuscluster_dec_bb.ecsv
plots/plots_limits/dmbounds/magic_2018_perseuscluster_dec_tautau.ecsv
plots/plots_limits/dmbounds/magic_2022_multidsph_ann_bb.ecsv
plots/plots_limits/dmbounds/magic_2022_multidsph_ann_tautau.ecsv
plots/plots_limits/dmbounds/veritas_2017_multidsph_ann_bb.ecsv
plots/plots_limits/dmbounds/veritas_2017_multidsph_ann_tautau.ecsv

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Additional titles

Alternative title
Data, notebooks

Related works

Is supplement to
Other: arXiv:2508.19120 (arXiv)

Software

Programming language
Python

References

  • @article{Abe:2025qsi, author = "Abe, K. and others", title = "{Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory}", eprint = "2508.19120", archivePrefix = "arXiv", primaryClass = "astro-ph.HE", month = "8", year = "2025" }