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CARMA
CARMA 225 GHz map with 0.9’’ beam (C-array)1’’ is not good enough!
BN?
source I
subarcsec resolution requires adaptive optics to correct for atmospheric blurring
blobs of water vapor
signal delayed to this antenna
differences from optical or NIR adaptive optics• water vapor fluctuations are the main problem• time scales of seconds, not milliseconds• no laser guide stars
paired antenna calibration (PACS)observe nearby calibrator at 30 GHz with 3.5-m antennas
3.5-m ant
quasar science target
paired antenna calibration in action
1mm B-array map before/after PACS corrections
BN
source I
229 GHz continuum map0.15’’ resolution
a reminder: interferometer acts as a spatial filter
H recombination lines toward BNRodriguez et al 2009 CARMA CARMA
CARMA SiO v=086.7 GHz, 0.4’’ res
SiO v=0 spectra suggest rotation about a NE-SW axis