Miriad is a radio interferometry data reduction package. Miriad can be configured for the specifications required by the Submillimeter Array (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 SMA data packed in Caltech's MIR format 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 which is managed by the BIMA group.

Questions: smamiriad@cfa.harvard.edu

• Miriad for SMA
• Miriad Users' Manual
• Specifications for the SMA
• Off-line Software Meeting

Three Major Milestones of SMA Miriad

• MiriadSWARMASIC (Miriad-SWARM 3.1.5 & higher)
• SWARM+ASIC data in new format¹
• ASIC (4GHz or 2GHz BW) data in new format¹


• Miriad4GHz (SMA-Miriad 1.5.1)
• ASIC data (4GHz or 2GHz BW)²
• Pre-processed SWARM+ASIC data in new format¹


• Miriad2GHz (Miriad-CVS 4.0.5)
• ASIC data (2GHz BW)³


• Report form: bugs & suggestions concerning SMA Miriad
• Q&A: 2019

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         ¹beyond 2014-11-15  ²prior to 2014-11-15  ³prior to 2009-11-30

Miriad for Other Telescopes:

• ATNF
• CARMA/BIMA
• IRAM (Gildas)
• WSRT