1. High Resolution Working Group
Andy Pollock Adam Foster

2. What is it?
Create a published line list using Chandra Capella spectrum
Compare with existing atomic databases

4. Actions from 2013

5. Actions from 2013
Progress: none

6. Actions from 2013
Progress: none

7. Now what? “The best is the enemy of good enough” Make a line list!
Observed wavelength, uncertainty
Lab wavelength, uncertainty
(Observed flux, estimated flux)

8. Expand targets Capella WR 140? HR 1099 Ar Lac Theta 1 Ori C
Vinay's Big List o' Stars(TM)

9. Now what? “The best is the enemy of good enough” Make a line list!
Assess uncertainties in line wavelengths in existing databases
Locate lines missing from databases
Search for DR satellite lines
Estimate missing flux from omitted line complexes
Diagnostics – list them, identify their reliability/quality/uncertainty

10. Bonus projects Study of calibration of existing instruments
Document what has been learned from calibration issues of current instruments.
What have we learned?
Which standards (in flight & on the ground) were most useful?
Interaction of analysis programs with calibration
How good does the cal need to be,
How good are packages at using it?

11. Shameless Plug!
6-9th September 2014
Tokyo
High-resolution spectroscopy workshop. Aimed at students/postdocs. Send yours!