Open keflavich opened 2 years ago
The continuum source in the top right corner is Sgr A*, so I don't think we will ever get a clean image without self calibration.
As @SpacialTree pointed out, spw 20 may have a problem in line-free channel identification, which leads to the odd dip in the first ~800 channels. The findcont result of spw 20:
The 'odd dip', seen in the mean spectrum in the mask in step 38:
The line-free mom8 of spw 20 shows features:
I checked the cube and it looks ok. The dip appears in the spectrum because the mask for plotting the spectrum happens to include one of the strong negative bowls around Sgr A*. Since we not use spw 20 for continuum imaging, and will probably do continuum subtraction in the image domain later, this should be fine...
spw20 spectrum in the hipergator pipeline run version (which uses 0th-order uvcontsub) looks better:
However, there are other issues in the hipergator pipeline run: spw24 diverged and spw26 is missing (could exist but missed by the weblog).
@SpacialTree could you do the reimaging for this field?
Going over the cubes in the products list:
Product Links:
No obvious issues with the baseline, multiple spectral lines visible.
No obvious issues with the baseline, interesting spectral feature shown in above image. Are the dips/absorption around the bright line typical or something that needs to be fixed?
Very complicated averaged spectrum. There's a sharp feature at 89.17.2821 GHz associated with a small part of the image
Other products are WIP for QA
No obvious issues with the baseline, lots of spectral lines
Similar issue to spw 20 where there are these sharp peaks associated with a small area of the image. There are 2-3 in this cube.
Major issues here. This cube has lots of teeth.
Major issues here. This cube has lots of teeth.
Gif showing the cube with the first section of the spectrum with the numerous strange peaks.
Re-imaged versions of these fields exist in /ACES/rawdata/science_goal.uid___A001_X1590_X30a8/group.uid___A001_X1590_X30a9/member.uid___A001_X15a0_X12c/calibrated/working/
. Not sure how to link directly to them, but they exist. They fixed the problem, but it doesn't seem like it was noted here? The links need to be updated above.
For spw 16, try uid___A001_X15a0_X12c.s12_0.Sgr_A_star_sci.spw16.cube.I.iter1.image.pbcor
For spw 18, try uid___A001_X15a0_X12c.s12_0.Sgr_A_star_sci.spw18.cube.I.iter1.image.pbcor
For spw 20, try uid___A001_X15a0_X12c.s12_0.Sgr_A_star_sci.spw20.cube.I.iter1.image.pbcor
For spw 22, try uid___A001_X15a0_X12c.s12_0.Sgr_A_star_sci.spw22.cube.I.iter1.image.pbcor
The \working\
images for spw 24 and spw 26 have issues, maybe do not use them.
@SpacialTree I am working on the feathering of CS2-1, and just post a channel of SPW 24 showing divergence.
Spw 24 divergence has been resolved.
Left = after reclean with cyclefactor = 3
. Right = before reclean
@SpacialTree thanks for the re-imaging, could you please upload the reclean files to /upload in Globus?
Re-imaged file for spw 24 has been uploaded to hipergator. I'm at UF so it was updated directly. Pull request for json file was made https://github.com/ACES-CMZ/reduction_ACES/pull/348 it just needs to be reviewed.
Sgr_A_st_x_03_7M uid://A001/X15a0/X12c
[x] Observations completed?
[x] Delivered?
[x] Downloaded? (specify where)
[ ] Weblog unpacked
[x] Weblog Quality Assessment?
Extra Weblog Sgr_A_st_x_03_7M_1 -> pipeline-20220715T140035, Extra Weblog Sgr_A_st_x_03_7M_0 -> pipeline-20220616T213105
[x] Imaging: Continuum
[x] Imaging: Lines
Product Links:
Reprocessed Product Links: