GOAL: disantangle between DMO based on stellar halo properties

2. Tue 15 Aug 10:52:18 CEST 2023

1. on se concentre que sur la halo
2. on garde tout pour r<75 kpc

DATA/stars_1keV_75kpc_n05.hdf5 DATA/stars_3keV_75kpc_n05.hdf5 DATA/stars_10keV_75kpc_n05.hdf5 DATA/stars_30keV_75kpc_n05.hdf5

1. 30.5 magnitudes correspond à env. 70 kpc/h (101 kpc) pour le halo
2. Quelle est la différence physique entre les 2 modèles ?

1. entre 50 et 60 kpc, on voit une différence (mais pas dans le bon ordre)
2. sur le profile de densité

./pSphericalProfile -o density --xmax 100 --rmax 100 --nr 256 --legend --log y \ DATA/stars_1keV_1000kpc_n05.hdf5 \ DATA/stars_3keV_1000kpc_n05.hdf5 \ DATA/stars_10keV_1000kpc_n05.hdf5 \ DATA/stars_30keV_1000kpc_n05.hdf5

./pSphericalProfile -o density --xmax 100 --rmax 100 --nr 256 --legend --log y \ DATA/stars_1keV_70kpc_n05.hdf5 \ DATA/stars_3keV_70kpc_n05.hdf5 \ DATA/stars_10keV_70kpc_n05.hdf5 \ DATA/stars_30keV_70kpc_n05.hdf5

2. brillance de area

mockimgs_sb_compute_images DATA/stars_1keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/1keV_VIS_CCD273-84_35Mpc.fits mockimgs_sb_compute_images DATA/stars_3keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/3keV_VIS_CCD273-84_35Mpc.fits mockimgs_sb_compute_images DATA/stars_10keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/10keV_VIS_CCD273-84_35Mpc.fits mockimgs_sb_compute_images DATA/stars_30keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/30keV_VIS_CCD273-84_35Mpc.fits

2. brillance de area pour model tronqué

mockimgs_sb_compute_images DATA/stars_1keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/1keV_VIS_CCD273-84_35Mpc_70kpc.fits mockimgs_sb_compute_images DATA/stars_3keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/3keV_VIS_CCD273-84_35Mpc_70kpc.fits mockimgs_sb_compute_images DATA/stars_10keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/10keV_VIS_CCD273-84_35Mpc_70kpc.fits mockimgs_sb_compute_images DATA/stars_30keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 1 -o fits/30keV_VIS_CCD273-84_35Mpc_70kpc.fits

./mockimgs_fits_manip fits/1keV_VIS_CCD273-84_35Mpc_70kpc.fits -o qq1keV.fits ./mockimgs_fits_manip fits/3keV_VIS_CCD273-84_35Mpc_70kpc.fits -o qq3keV.fits ./mockimgs_fits_manip fits/10keV_VIS_CCD273-84_35Mpc_70kpc.fits -o qq10keV.fits ./mockimgs_fits_manip fits/30keV_VIS_CCD273-84_35Mpc_70kpc.fits -o qq30keV.fits

ds9 qq1keV.fits qq3keV.fits qq10keV.fits qq30keV.fits

./mockimgs_fits_histogram qq1keV.fits qq3keV.fits qq10keV.fits qq30keV.fits

"halo" plus étendu ? (/home/revaz/Projects/ARRAKIHS/repo/arrakihs/ParticlesToareaBrightness/arrakihs_compute_illuminated.py)

./mockimgs_fits_compute_area \ fits/1keV_VIS_CCD273-84_35Mpc_70kpc.fits \ fits/3keV_VIS_CCD273-84_35Mpc_70kpc.fits \ fits/10keV_VIS_CCD273-84_35Mpc_70kpc.fits \ fits/30keV_VIS_CCD273-84_35Mpc_70kpc.fits

1. multiple images
2. limit to 70kpc

mockimgs_sb_compute_images DATA/stars_1keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/1keV_VIS_CCD273-84_35Mpc_70kpc.pkl mockimgs_sb_compute_images DATA/stars_3keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/3keV_VIS_CCD273-84_35Mpc_70kpc.pkl mockimgs_sb_compute_images DATA/stars_10keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/10keV_VIS_CCD273-84_35Mpc_70kpc.pkl mockimgs_sb_compute_images DATA/stars_30keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/30keV_VIS_CCD273-84_35Mpc_70kpc.pkl

./mockimgs_pkl_compute_area \ pkl/1keV_VIS_CCD273-84_35Mpc_70kpc.pkl \ pkl/3keV_VIS_CCD273-84_35Mpc_70kpc.pkl \ pkl/10keV_VIS_CCD273-84_35Mpc_70kpc.pkl \ pkl/30keV_VIS_CCD273-84_35Mpc_70kpc.pkl

1. multiple images
2. no limit

mockimgs_sb_compute_images DATA/stars_1keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/1keV_VIS_CCD273-84_35Mpc.pkl mockimgs_sb_compute_images DATA/stars_3keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/3keV_VIS_CCD273-84_35Mpc.pkl mockimgs_sb_compute_images DATA/stars_10keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/10keV_VIS_CCD273-84_35Mpc.pkl mockimgs_sb_compute_images DATA/stars_30keV_1000kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/30keV_VIS_CCD273-84_35Mpc.pkl

./mockimgs_pkl_compute_area \ pkl/1keV_VIS_CCD273-84_35Mpc.pkl \ pkl/3keV_VIS_CCD273-84_35Mpc.pkl \ pkl/10keV_VIS_CCD273-84_35Mpc.pkl \ pkl/30keV_VIS_CCD273-84_35Mpc.pkl

2. Check is the orientation has an influence on the
3. extension of the halo

in "aligned/"

cp

glups -> self.nb.align_with_main_axis()

self.nb.rotate(axis='y',angle=np.pi/2)

-> estimate the size of the halo

mockimgs_sb_compute_images aligned/stars_1keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 0 1 0 -o qq_1.fits mockimgs_sb_compute_images aligned/stars_3keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 0 1 0 -o qq_2.fits mockimgs_sb_compute_images aligned/stars_10keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 0 1 0 -o qq_3.fits mockimgs_sb_compute_images aligned/stars_30keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 0 1 0 -o qq_4.fits

mockimgs_sb_compute_images aligned/stars_1keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 1 0 0 -o qq_1.fits mockimgs_sb_compute_images aligned/stars_3keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 1 0 0 -o qq_2.fits mockimgs_sb_compute_images aligned/stars_10keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 1 0 0 -o qq_3.fits mockimgs_sb_compute_images aligned/stars_30keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --los 1 0 0 -o qq_4.fits

mockimgs_sb_compute_images aligned/stars_1keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o qq.fits

./mockimgs_fits_compute_area qq_1.fits qq_2.fits qq_3.fits qq_4.fits

mockimgs_sb_compute_images aligned/stars_1keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/1keV_VIS_CCD273-84_35Mpc.pkl mockimgs_sb_compute_images aligned/stars_3keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/3keV_VIS_CCD273-84_35Mpc.pkl mockimgs_sb_compute_images aligned/stars_10keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/10keV_VIS_CCD273-84_35Mpc.pkl mockimgs_sb_compute_images aligned/stars_30keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 --nlos 9 -o pkl/30keV_VIS_CCD273-84_35Mpc.pkl

./mockimgs_pkl_compute_area \ pkl/1keV_VIS_CCD273-84_35Mpc.pkl \ pkl/3keV_VIS_CCD273-84_35Mpc.pkl \ pkl/10keV_VIS_CCD273-84_35Mpc.pkl \ pkl/30keV_VIS_CCD273-84_35Mpc.pkl

estimate a dispersion along a given axis

mockimgs_sb_compute_images aligned/stars_1keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 -p params.yml -o pkl/1keV_VIS_CCD273-84_35Mpc_EO20.pkl mockimgs_sb_compute_images aligned/stars_3keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 -p params.yml -o pkl/3keV_VIS_CCD273-84_35Mpc_EO20.pkl mockimgs_sb_compute_images aligned/stars_10keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 -p params.yml -o pkl/10keV_VIS_CCD273-84_35Mpc_EO20.pkl mockimgs_sb_compute_images aligned/stars_30keV_70kpc_n05.hdf5 --instrument arrakihs_vis_GAIA_VIS --distance 35 -p params.yml -o pkl/30keV_VIS_CCD273-84_35Mpc_EO20.pkl

./mockimgs_pkl_compute_area $SCRATCH/pkl/*keV_VIS_CCD273-84_35Mpc_EO10.pkl