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fluxes_script [2012/06/07 23:11] – [flux (driver function)] amberbfluxes_script [2012/06/07 23:14] – [Quick Overview] amberb
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 ======Quick Overview====== ======Quick Overview======
 ===The Process=== ===The Process===
-  - Remove bad windows for sci2/CARMA23 obs (from original vis file) -> **vis_sci2.mir** +  - Extract spectral channels only (from original vis file) -> **speconly.mir** 
-  - Just wide-band windows, pol(LL) (from original vis or vis_sci2.mir) -> **wb.mir**+  - Remove bad windows for sci2/CARMA23 obs (from speconly.mir) -> **vis_sci2.mir** 
 +  - Just wide-band windows, pol(LL) (from speconly.mir or vis_sci2.mir) -> **wb.mir**
   - Amplitude flagging creates intermediate files described below, but flags wb.mir. (These steps made necessary because smauvplt cannot average if there is a planet in the observation...reason unknown)   - Amplitude flagging creates intermediate files described below, but flags wb.mir. (These steps made necessary because smauvplt cannot average if there is a planet in the observation...reason unknown)
     - planet-only uvmodel options=divide -> **wb_planet.mir**     - planet-only uvmodel options=divide -> **wb_planet.mir**

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