SMA Mauna Kea

SMA




Miriad is a radio interferometry data reduction package. Miriad can be configured for the specifications required by the SMA. Specific codes for handling the SMA data have been developed and are supported. Miriad now can be used for the reduction of continuum and spectral line observations from loading of the original SMA data (Caltech's MIR formats) through to the image analysis.

The SMA features have particular emphasis on aspects of interest to users of the SMA. We support the off-line software including software tools used for calibration and analysis of the SMA data observed at submillimeter wavelengths. The newly developed codes are (will be) placed under Miriad CVS system (./miriad_cvs/src/prog/sma) which is managed by the BIMA group.



Ram Rao (SAO), Shengyuan Liu (ASIAA), Peter Teuben (Maryland), Bob Wilson (SAO), Mel Wright (Berkeley) and Jun-Hui Zhao (SAO)

Questions: smamiriad@cfa.harvard.edu

MIRIAD for SMA

Miriad Users' Manual

Specifications for SMA

CVS Tutorial

Minutes of SMA Offline Software (Miriad) Meeting

Miriad for Other Telescopes: ATNF , CARMA/BIMA , IRAM (Gildas) , WSRT