Phase Corrections at the OVRO Millimeter Array using
Atmospheric Water Vapor Observations
John Carpenter (Caltech), Dave Woody (OVRO), and Nick Scoville (Caltech)
Table of Contents
Introduction
The Water Line Monitors
Example water line data
Results for Individual Tracks
Correlation between WLM and Phase
Before/After images
Viewgraphs from URSI Conference
How to Apply the WLM corrections to your data --- INCOMPLETE
Writing schedule files to use the WLM corrections --- INCOMPLETE
Recent bug fixes in IDL code
Coming soon...
WLM corrections at 1mm
Before/after images
John Carpenter
jmc@astro.caltech.edu
Last modified: Mon April 1, 1999