Closed bjfultn closed 7 years ago
I ran GL699 (Barnard's Star) for both APF and Keck.
APF velocities vs. BC (poor coverage): iGrand_GL699_bcbyiter.pdf
Keck velocities vs. BC (CPS RMS = 2.5 m/s): iGrand_GL699_bcbyiter.pdf
Keck template evolution plots: iGrand_GL699_02_temp_byiter.pdf iGrand_GL699_03_temp_byiter.pdf iGrand_GL699_04_temp_byiter.pdf iGrand_GL699_05_temp_byiter.pdf iGrand_GL699_06_temp_byiter.pdf iGrand_GL699_07_temp_byiter.pdf iGrand_GL699_08_temp_byiter.pdf iGrand_GL699_09_temp_byiter.pdf iGrand_GL699_10_temp_byiter.pdf iGrand_GL699_11_temp_byiter.pdf
APF template evolution plots: iGrand_GL699_02_temp_byiter.pdf iGrand_GL699_03_temp_byiter.pdf iGrand_GL699_04_temp_byiter.pdf iGrand_GL699_05_temp_byiter.pdf iGrand_GL699_06_temp_byiter.pdf iGrand_GL699_07_temp_byiter.pdf iGrand_GL699_08_temp_byiter.pdf iGrand_GL699_09_temp_byiter.pdf iGrand_GL699_10_temp_byiter.pdf iGrand_GL699_11_temp_byiter.pdf iGrand_GL699_12_temp_byiter.pdf iGrand_GL699_13_temp_byiter.pdf
Send Jay Keck GL699 spectra
Jay says that template convergence is not working well for Mdwarfs.
APF RMS is a factor of ~2 better than before with the more finely sampled template. Still shows some systematics with BC, but BC phase coverage is poor.
Keck is looking much better and approaching the 2.5 m/s RMS of the CPS code.
Order 2 is performing very poorly, but I suspect it is not affecting the final results too much because of the weighting scheme. iGrand_GL699_bcbyord.pdf
Run a small sample of Mdwarfs from both Keck and APF with high SNR observations.