Radio Astronomy Interest Group ( Jointly organised with Data Model Working Group)Eight Virtual Running Meeting 2024, July 2nd via zoom15:30 to 16:30 UTCZoom coordinates: https://astron.zoom.us/j/81533464364?pwd=bQh0hVs3x3kAmjaLbwoDNJsjIFyIWS.1 Meeting ID: 815 3346 4364 Passcode: 354277 Telecon Agenda: | ||||||||
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< < | 1) Representation of the ObsCore extension: | |||||||
> > | 1) Representation of the ObsCore extension: | |||||||
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< < | The PR standardizes a new ivoa.obscore_radio table and mandates the presence of a obs_publisher_did column in order to be able to do a NATURAL JOIN. Note that Markus suggested to not specify an explicit column to join on... | |||||||
> > | The PR standardizes a new ivoa.obscore_radio table and mandates the presence of a obs_publisher_did column in order to be able to do a NATURAL JOIN. Note that Markus suggested to not specify an explicit column to join on... | |||||||
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< < | The PR suggests the possibility to provide a view that does that performs this join but doesn't mandate it and doesn't provide a standardized name for it. Is this desirable? Should this be standardized? How would this work for combining multiple extensions (i.e. Radio + Time Domain). | |||||||
> > | The PR suggests the possibility to provide a view that does that performs this join but doesn't mandate it and doesn't provide a standardized name for it. Is this desirable? Should this be standardized? How would this work for combining multiple extensions (i.e. Radio + Time Domain). | |||||||
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< < | 2) Discovery of ObsCore extensions | |||||||
> > | 2) Discovery of ObsCore extensions | |||||||
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< < | Converged on using a utype, but there are still multiple suggestions for the name (ivo://ivoa.net/std/obsradio#table-1.0 vs. ivo://ivoa.net/std/ObsCore#obscore-radioExt-1.0) ? | |||||||
> > | Converged on using a utype, but there are still multiple suggestions for the name (ivo://ivoa.net/std/obsradio#table-1.0 vs. ivo://ivoa.net/std/ObsCore#obscore-radioExt-1.0) ? | |||||||
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< < | Should we introduce both table_utype and schema_utype for extensions? | |||||||
> > | Should we introduce both table_utype and schema_utype for extensions? | |||||||
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< < | 3) t_exp_{min|max|mean} | |||||||
> > | 3) t_exp_{min|max|mean} | |||||||
These still need a science case in the Appendix. Can someone (Baptiste?) provide one? Naming is somewhat confusing (name is similar to t_exptime in ObsCore, but describing a different concept)? Is the description correct now? | ||||||||
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< < | 4) s_maximum_angular_scale_{min|max} | |||||||
> > | 4) s_maximum_angular_scale_{min|max} | |||||||
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< < | Like the FOV and resolution, the maximum spatial scale is actually frequency-dependent. Should we include min/max values in addition to a typical value? | |||||||
> > | Like the FOV and resolution, the maximum spatial scale is actually frequency-dependent. Should we include min/max values in addition to a typical value? | |||||||
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< < | 5) f_{min|max} | |||||||
> > | 5) f_{min|max} | |||||||
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< < | These have been dropped in the PR. How to convert em_{max|min} into frequencies has been specified in the standard with a prescribed value for the speed of light. f_resolution has been retained to cater for observations with large fractional bandwidth and fixed spectral resolution across the band. Settled? | |||||||
> > | These have been dropped in the PR. How to convert em_{max|min} into frequencies has been specified in the standard with a prescribed value for the speed of light. f_resolution has been retained to cater for observations with large fractional bandwidth and fixed spectral resolution across the band. Settled? | |||||||
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< < | 6) Next steps | |||||||
> > | 6) Next steps | |||||||
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< < | Are we ready for RFC phase? | |||||||
> > | Are we ready for RFC phase? | |||||||
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< < | 7) AOB | |||||||
> > | 7) AOB | |||||||
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Recording:https://drive.google.com/file/d/1OvfKgpM2go8oXY4NVNajTkPnbiXyIYd5/view?usp=share_link | |||||||
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