Differences
This shows you the differences between two versions of the page.
| Both sides previous revisionPrevious revision | Next revisionBoth sides next revision | ||
| fluxcal_notes [2012/06/06 17:22] – amberb | fluxcal_notes [2012/06/06 17:35] – [Telecon, Jun 6] amberb | ||
|---|---|---|---|
| Line 11: | Line 11: | ||
| * Peter: | * Peter: | ||
| * new model from Brian Butler on Mars - Jan 2010 - Dec 2020 in 1 hour intervals at 30-1000 GHz (this is becoming the standard model in CASA) - 11 MB | * new model from Brian Butler on Mars - Jan 2010 - Dec 2020 in 1 hour intervals at 30-1000 GHz (this is becoming the standard model in CASA) - 11 MB | ||
| - | * miriad program marstb will be able to read this soon - use table= to read 1hr cadence | + | * miriad program marstb will be able to read this soon - use table= to read 1hr cadence |
| + | * Uranus and Neptune models - European + North American collaboration. Hofstader model is more appropriate at 1cm, but this model is better at 3mm and 1mm. | ||
| * fluxcal on science: | * fluxcal on science: | ||
| * copy could take a minute or two but it does happen all in one go - check size of visdata | * copy could take a minute or two but it does happen all in one go - check size of visdata | ||
| - | * multiple corr configs - | + | * multiple corr configs - Doug: sci1 track doppler tracking wasn't set up in first NOISE integration - this is nothing to worry about. sci2...?? wideband channels have a bandwidth of 0...maybe first antenna is being flagged by the system. maybe try re-running uvwide to recalculate the wideband channels from the spectral line channels. uvcat just spectral channels out options=nowide. |
| + | * Andreea - looking for comments on everything (incorporated my comments) | ||
| ===== Telecon, May 30 ===== | ===== Telecon, May 30 ===== | ||
