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open:wp4:wp4techforum5:radiointhevo [2019/03/13 16:20] bonnarel |
open:wp4:wp4techforum5:radiointhevo [2019/03/13 16:21] (current) bonnarel |
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| I ) **status and feedback on Multi-D and existing standard protocols for radio data** | I ) **status and feedback on Multi-D and existing standard protocols for radio data** | ||
| ObstPAP(Obscore)-SIAV2+DataLink+SODA+clients(Aladin) work for imaging cubes (science ready | ObstPAP(Obscore)-SIAV2+DataLink+SODA+clients(Aladin) work for imaging cubes (science ready | ||
| - | products) | + | products) |
| HiPS works for the same (full 3D HiPS or alternatively 2D continuum HiPS + DataLink access | HiPS works for the same (full 3D HiPS or alternatively 2D continuum HiPS + DataLink access | ||
| - | to cubes, Other moment maps SODA). See CASDA (ASKAP) data + partially ALMA. Detailed | + | to cubes, Other moment maps SODA). See CASDA (ASKAP) data + partially ALMA. Detailed |
| analysis by INAF. | analysis by INAF. | ||
| MOC also useful for discovery. But MOC in velocity could help. | MOC also useful for discovery. But MOC in velocity could help. | ||
| Due to the nature of raw data, image sensitivity may change a lot from pixel to pixel .. | Due to the nature of raw data, image sensitivity may change a lot from pixel to pixel .. | ||
| - | --> need for sensitivity cubes? | + | --> need for sensitivity cubes? |
| Some of the data are complex. ObsCore not really suited for this. Use of CAOM better? | Some of the data are complex. ObsCore not really suited for this. Use of CAOM better? | ||
| Coarse grain discovery of raw data (or calibrated discovery) via ObstAP/SIAV2 (or HiPS + | Coarse grain discovery of raw data (or calibrated discovery) via ObstAP/SIAV2 (or HiPS + | ||
| - | DataLink) probably possible, but not experimented yet. Links to project native pages for | + | DataLink) probably possible, but not experimented yet. Links to project native pages for |
| - | the data can be made available | + | the data can be made available |
| It appears that currently most of the data in the radio archives are not science ready. | It appears that currently most of the data in the radio archives are not science ready. | ||
| - | So there is a big question mark: why and how integrating visibility/raw data in the VO? | + | So there is a big question mark: why and how integrating visibility/raw data in the VO? |