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| fluxcal_notes [2012/06/06 17:22] – amberb | fluxcal_notes [2012/06/13 17:13] – amberb | ||
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| * Figure out algorithm for error estimation (currently 15%, or RMS of values) | * Figure out algorithm for error estimation (currently 15%, or RMS of values) | ||
| * check that planet brightness temp is different for different windows | * check that planet brightness temp is different for different windows | ||
| + | |||
| + | ===== Telecon, Jun 13 ===== | ||
| + | * online: Amber, Statia, Woojin, Manuel, Doug, Peter | ||
| + | * data transfer issue at Illinois: | ||
| + | * issue with script | ||
| + | * Peter - testing new code with Woojin | ||
| + | * 3 mars tables: | ||
| + | * 1 is marstb original increments of 25 days | ||
| + | * 2 is marstb2 stops at 115 GHz, increments of 6 hours | ||
| + | * 3 is marstb3 1cm to 260 GHz, increments of 1 hours | ||
| + | * this table is ~5 K cooler than old curves at 115 GHz - see Woojin' | ||
| + | * need to check at other freq and if spec index is the same, then ask Brian Butler | ||
| + | * can play with these in new miriad - marstb with table= (need to grab tar files for the tables first) | ||
| + | * will build new binaries for school students tomorrow but it is in CVS now | ||
| + | * fluxtest script is in Miriad now | ||
| + | * | ||
| ===== Telecon, Jun 6 ===== | ===== Telecon, Jun 6 ===== | ||
| Line 11: | Line 27: | ||
| * 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 ===== | ||
