summary

//Remarks: Zhong, would you please update your tracks' status here?//
 * ====Project Code==== || ====Object==== || ====Frequency (GHz)==== || ====Configuration==== || ====Observed?==== || ====Status==== ||
 * 09A-H007 || NGC6240 || 345 || VEX || 20090705 || Data reduced and mapped; see object page ||
 * 09A-S071 || NGC1614 || 230 || EXT || 20090831 || Data reduced and mapped; see object page ||
 * || IR17208 || 230 || EXT || 20090821 || Data reduced and mapped; see object page ||
 * || IC1623 || 230 || EXT || 20090810 || Data downloaded ||
 * || IR19297 || 230 || COM || 20090613 || Data downloaded ||
 * || IR05189 || 230 || COM || not observed ||  ||
 * || IR21101 || 230 || COM || not observed ||  ||
 * || ESO593 || 230 || COM || not observed ||  ||
 * 09B-H003 || UGC5101 || 345 || VEX || 20100207 || Data processed crudely; no obvious line? ||
 * || NGC2623 || 230 || VEX || 20100215 || Data processed crudely; no obvious line? ||
 * || UGC8058 || 230 || VEX || 20100307 || Data processed crudely; wide line? ||
 * 09B-H008 || UGC8696 || 230 || VEX || not observed ||  ||
 * || UGC4881 || 230 || VEX || not observed ||  ||
 * 09B-S074 || IR17578 || 230 || COM || 20100509 || Zhong? ||
 * || NGC6786 || 230 || COM || 20100507 || Zhong? ||
 * || CGCG436-030 || 230 || COM || not observed ||  ||
 * 10A-S063 || IR03359 || 345 || EXT || in queue ||  ||
 * || IR17132 || 345 || EXT || in queue ||  ||
 * 10A-H008 || IR17132 || 345 || VEX || 20100717 || Data obtained ||
 * || IR17208 || 345 || VEX || 20100727 || Data obtained ||
 * || NGC6090 || 345 || VEX || 20100723 || Data obtained ||
 * || CGCG448-020 || 345 || VEX || 20100720 || Data obtained ||
 * 10B-S062 || NGC2623 || 230 || VEX || 20110110 || Data obtained ||
 * || UGC04881 || 230 || VEX || 20110115 || Data obtained ||
 * || UGC05101 || 230 || VEX || in queue ||  ||
 * 10B-S100 || IC694 || 230 || EXT || 20110212 || Europa - not the best flux calibrator (GP) ||
 * || NGC 3690 || 230 || EXT || 20110215 || Tau got better over 2 tracks - use both? ||

**Future Plans**
This project has essentially split into two complementary directions: 1. The high-resolution study aims for "very extended" configuration observations to look at the centers of a small sample of (U)LIRGs which have previous lower-resolution interferometric maps, mainly from the Wilson et al. 2008 SMA studies; 2. The lower-resolution study aims for "compact" configuration observations as an expansion of the Wilson et al. 2008 comprehensive study of the local (U)LIRGs so to prepare for higher-resolution interferometric observations.

Also as a preparation step for interferometric observations, some CO(2-1) and CO(3-2) line data have been taken at JCMT in Sept 2009 for a sample of (lower luminosity) LIRGs that have not been observed in CO previously.

Reference

 * Wilson et al. 2008, ApJS, 178, 189