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ACES-CMZ / reduction_ACES

Reduction scripts and tools for ACES
https://worldwidetelescope.org/webclient/?wtml=https://data.rc.ufl.edu/pub/adamginsburg/ACES/mosaics/mosaics.wtml
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Execution Block ID uid://A001/X15a0/X136 Sgr_A_st_z_03_TM1 #131

Open keflavich opened 2 years ago

keflavich commented 2 years ago

Sgr_A_st_z_03_TM1 uid://A001/X15a0/X136

Product Links:

Reprocessed Product Links:

d-l-walker commented 2 years ago

Everything looks good here, no obvious issues. SPW 33 needs to be imaged, as it was dropped for size mitigation as usual. Once this has been done, I think this is a clear pass.

There's some residual emission in the line-free mom8 image for SPW 29. Could be reduced with refined continuum channel selection, but this is very minor.

d-l-walker commented 2 years ago

SPW 33 was successfully imaged by the PL re-run and it looks good, so I'm setting this one as 'Done' since that was the only outstanding issue.

Screenshot 2022-08-03 at 12 06 36

ksi85 commented 8 months ago

QA - Line contamination in continuum images from high/low frequencies

Summary: looks ok to me

Files checked:

New: spw25_27 and spw33_35 Old: spw25_27_29_31_33_35 and oldhigh_spw33_35 Results: New continuum images look good

Attached image:

Top-left: spw25_27_29_31_33_35 Top-right: spw25_27 Bottom-left: oldhigh_spw33_35 Bottom-right: spw33_35

Continuum

ksi85 commented 7 months ago

QA - Line contamination in continuum images from high/low frequencies version 2 (Apr2024)

Summary: looks ok to me

Files checked:

New: spw25_27 and spw33_35 Old: spw25_27_29_31_33_35 and oldhigh_spw33_35 Results: New continuum images look good

Attached image:

Top-left: spw25_27_29_31_33_35 Top-right: spw25_27 Bottom-left: oldhigh_spw33_35 Bottom-right: spw33_35

Continuum_new