Supplementary material of CTAO publication "Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory "
Authors/Creators
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 details
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" }