Closed cbischoff closed 4 years ago
There seems to be something funny about the input maps. The dust input map is /global/cscratch1/sd/zonca/cmbs4/map_based_simulations/202006_foregrounds_extragalactic_cmb_tophat/512/dust/0000/cmbs4_dust_uKCMB_SAT-HFS2_nside512_0000.fits
and, like you said, it should form the bulk of the combined foreground map at /global/cscratch1/sd/zonca/cmbs4/map_based_simulations/202006_foregrounds_extragalactic_cmb_tophat/512/combined_foregrounds/0000/cmbs4_combined_foregrounds_uKCMB_SAT-HFS2_nside512_0000.fits
.
Here are some standard deviations measured in dust
and combined_foregrounds
:
| full sky | SAT HFS2 patch
| I | Q | U | I | Q | U |
dust | 3241 | 59.3 | 28.0 | 131.1 | 6.3 | 5.4 |
combined_foregrounds | 3309 | 61.1 | 31.5 | 138.1 | 15.7 | 15.4 |
combined_foregrounds - dust | 93.9 | 14.4 | 14.4 | 17.7 | 14.4 | 14.4 |
So the combined foreground polarization in the SAT patch at HFS2 is dominated by something entirely different than dust. What do you think it is @zonca ?
Found it! The CIB component in /global/cscratch1/sd/zonca/cmbs4/map_based_simulations/202006_foregrounds_extragalactic_cmb_tophat/512/cib/0000/cmbs4_cib_uKCMB_SAT-HFS2_nside512_0000.fits
has exactly same map in the I, Q and U columns of the FITS file. The standard deviation also matches the 14.4uK excess we saw above.
sorry, I noticed something in the CIB, see https://github.com/CMB-S4/s4mapbasedsims/issues/3, but haven't investigate yet.
there was a wrong broadcasting, so CIB which is T only was replicated on polarization as well.
I have rerun the SAT and generated CIB and the combined map again, can you please rerun your checks on these? Currently are on my scratch, if they are fine I'll run on LAT and copy to the project folder.
/global/cscratch1/sd/zonca/cmbs4/map_based_simulations/202006_foregrounds_extragalactic_cmb_tophat/512/cib/0000
/global/cscratch1/sd/zonca/cmbs4/map_based_simulations/202006_foregrounds_extragalactic_cmb_tophat/512/combined_foregrounds/0000
Yes, this looks much improved. Just to check, the CIB component is now totally unpolarized?
Yes, Q and U are 0 arrays
The new Pole SAT maps are here: /global/cscratch1/sd/keskital/s4sim/reference_tool/out_v2
.
ok, I regenerated the foregrounds
outputs at: /global/cscratch1/sd/zonca/cmbs4/s4refsimtool/s4_reference_design_foregrounds
if they are fine I'll copy to project
@zonca When will you have the LAT foreground maps prepared?
I'm trying on Jupyter, if that works, tonight, if not, Monday night
@keskitalo ok, LAT maps are available at /global/cscratch1/sd/zonca/cmbs4/map_based_simulations/202006_foregrounds_extragalactic_cmb_tophat/4096/combined_foregrounds/0000
All of the filtered foreground maps can be found here: /global/cscratch1/sd/keskital/s4sim/reference_tool/out_v2
thanks @keskitalo
LAT output maps are at /global/cscratch1/sd/zonca/cmbs4/s4refsimtool/s4_reference_design_foregrounds
I will run some validation and then copy everything to project, please write here if you have any more feedback.
Just to get us all in the right habits, we're actually running verification (did we do the thing right) on the maps now, not validation (did we do the right thing).
Julian
On Mon, Aug 10, 2020 at 9:40 AM Andrea Zonca notifications@github.com wrote:
thanks @keskitalo https://github.com/keskitalo
LAT output maps are at /global/cscratch1/sd/zonca/cmbs4/s4refsimtool/s4_reference_design_foregrounds
I will run some validation and then copy everything to project, please write here if you have any more feedback.
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@jdborrill correct, thanks
/global/project/projectdirs/cmbs4/dm/dstool/input_pysm
with the LAT and SAT fixed cib
and combined_foregrounds
/global/project/projectdirs/cmbs4/dm/dstool/input/00000000
/global/project/projectdirs/cmbs4/dm/dstool/output/s4_reference_design_foregrounds
, just in case saved the old one as /global/project/projectdirs/cmbs4/dm/dstool/output/s4_reference_design_foregrounds_broken_cib
added gnomview
plots to check consistency of input and output foregrounds: https://github.com/CMB-S4/s4mapbasedsims/blob/master/202006_reference_design/plot_gnomview/README.md
ok, this is completed, I posted link to the DM reference sims docs on the sim and analysis logbook: https://cmb-s4.org/wiki/index.php/Simulation_and_Forecasting_Logbook#Logbook_Entries_.28reverse_chronological.29
dstool/input_pysm/512/dust/0000/cmbs4_dust_uKCMB_SAT-HFS2_nside512_0000.fits
dstool/output/s4_reference_design_foregrounds/SAT-HFS2_pole/cmbs4_KCMB_SAT-HFS2_pole_nside512_1_of_1.fits
-- since we are at 270 GHz, this map should be primarily dust.dstool/output/s4_reference_design_noise_atmo_7splits/SAT-HFS2_pole/cmbs4_hitmap_SAT-HFS2_pole_nside512_1_of_1.fits
), then visually compare the Q/U maps. There is no obvious visual correlation and the cross-spectrum between the two maps bounces around zero. The output Q/U foreground maps have ~3x larger amplitude with power weighted towards small scales.