00:14:15	Meredith MacGregor:	Welcome everyone!  A few instructions for how the webinar will work today:
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00:50:36	Wanggi Lim:	I presume you can derive the column densities of individual molecules. Could you have time to look for the abundance ratios of those comparing to hydrogen?
00:51:20	Ryan Fortenberry:	Question for Sara: Why not include isolated (not crystalline) SiO2, as well?
00:52:43	Ryan Fortenberry:	Okay, that’s fine.
00:55:02	Ryan Fortenberry:	Thanks, Sarah!  Sorry you had to deal with the zoom-bombers.
00:55:03	David Dubois:	thank you Sarah!
00:55:09	Randolf Klein:	Thanks!
00:55:11	nrangwal:	Great Talk Sarah! :)
00:55:12	Alexandre Marciniak:	thanks
00:55:17	nrangwal:	Thanks Meredith!
00:55:17	Bernhard Schulz:	Thanks, nice talk!
00:55:21	Wanggi Lim:	Thank you so much!
00:55:21	zemcov:	Thanks Sarah!
00:55:30	Alwyn Wootten:	Thanks!
00:55:34	Fatemeh Hasheminasab:	thank you for nice presentation
00:55:35	Robert Minchin:	Thanks Sarah
00:56:11	cdewitt:	In answer to Berhard’s question, The TEXES /IRTF archive has a lot unpublished  data for NH3 800-900cm-1, and CS/SiO 1200-1300cm-1. Also a selection of the C2H2 and HCN lines that have slipped through the windows in the atmosphere.