Execution Block ID uid://A001/X15a0/Xc6 Sgr_A_st_g_03_7M

[keflavich]

Sgr_A_st_g_03_7M uid://A001/X15a0/Xc6

• [x] Observations completed?

• [x] Delivered?

• [x] Downloaded? (specify where)

  • [x] hipergator
  • [x] hipergator pipeline run
  • Pipeline Run 20220708T164046
  • Pipeline Run 20220708T173715
  • Pipeline Run 20220709T040735

• [ ] Weblog unpacked

• [x] Weblog Quality Assessment?

• Extra Weblog Sgr_A_st_g_03_7M_0 -> pipeline-20220709T040735, Extra Weblog Sgr_A_st_g_03_7M_1 -> pipeline-20220623T194044

• [x] Imaging: Continuum

• [x] Imaging: Lines

  • [x] SPW16 H13CN
  • [x] SPW18 H13CO+/SiO
  • [x] SPW20 HCO+
  • [x] SPW22 HNCO
  • [x] SPW24 Cont 1
  • [x] SPW26 Cont 2

Product Links:

Reprocessed Product Links:

• uid___A001_X15a0_Xc6.s8_0.Sgr_A_star_sci.spw18.mfs.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s8_0.Sgr_A_star_sci.spw24.mfs.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s8_0.Sgr_A_star_sci.spw20.mfs.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s8_0.Sgr_A_star_sci.spw22.mfs.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s8_0.Sgr_A_star_sci.spw26.mfs.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s8_0.Sgr_A_star_sci.spw16.mfs.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s12_0.Sgr_A_star_sci.spw20.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s12_0.Sgr_A_star_sci.spw18.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s12_0.Sgr_A_star_sci.spw16.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s38_0.Sgr_A_star_sci.spw22.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s38_0.Sgr_A_star_sci.spw18.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s38_0.Sgr_A_star_sci.spw24.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s38_0.Sgr_A_star_sci.spw26.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s36_0.Sgr_A_star_sci.spw16_18_20_22_24_26.cont.I.iter1.image.tt0.pbcor.fits
• uid___A001_X15a0_Xc6.s38_0.Sgr_A_star_sci.spw24.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s38_0.Sgr_A_star_sci.spw26.cube.I.iter1.image.pbcor.fits
• uid___A001_X15a0_Xc6.s38_0.Sgr_A_star_sci.spw22.cube.I.iter1.image.pbcor.fits

[d-l-walker]

Data look good, no significant issues. Once the HPG PL has finished running I think this can go straight to 'Done'. Some minor things to note:

• Continuum could be cleaned deeper.
• Very few continuum channels in SPWs 20 & 22. Looks like there might be a slight slope in the spectrum for SPW 20, but this should be fixed when running the PL with fitorder=0.
• Warning that "tclean reached niter limit of 199999 for Sgr_A_star / spw22 / iter1 !". This isn't a problem, but it could be cleaned a bit deeper (as could most SPWs).

[d-l-walker]

The PL has done several re-runs here, and the spectrum for SPW 20 looks better now in the 20220709T040735 run (no slope). Unfortunately the PL run only cleaned SPWs 16 & 20, and the others failed with the usual generic error.

Given that there are no actual issues to be resolved here, should I set this to 'Done' even though the PL re-runs failed?

[keflavich]

If the data are OK in their present state, yes.