Differences
This shows you the differences between two versions of the page.
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fluxes_script [2012/06/07 23:11] amberb [flux (driver function)] |
fluxes_script [2012/06/07 23:14] (current) amberb [Quick Overview] |
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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** | ||
