2017-06-20 09:47:59 +00:00
2017 grids needed
mehdipour SED, solar, 10²² - 10²⁴
magdziarz SED, solar, 10²² - 10²⁴
magdziarz SED, metals 0.5 & element scale factor carbon 2, 10²² - 10²⁴
2017-03-29 08:46:09 +00:00
By end of March: two grids run, continuum points decided upon, models decided upon
Run grid with new SED, or at least a point, check values: how to find the appropriate values to change our list accordingly, and what might need to be change?
2017-05-02 05:04:17 +00:00
✓ faint to equivalent width of 0.01 angstrom
✓ compare between c13 and c17 -- show diferences in emergent line lists
✓ new print lines to help reduce number of printed lines -- and to show old lines?
✓ run models for comparising: 10.5,19.5
□ Why so many Fe 2 lines?
□ check if blnds are sums of the expected multiplets
□ add in more levels to the H atom, unresolved, 20, also add some to paschen, maybe others -- check how much time is lost
□ punch the paschen and balmer lines up to 18
2017-05-08 13:13:23 +00:00
□ Read Intrinsic Lines
□ Smoothing algorithm using n-dimensional smoothing
□ Contour plots
□ Run Grids in c17
□ Email about order of lines
□ Find blend correlated names and update
2017-05-02 05:04:17 +00:00
check on ratios of inwd lines for blends
check hazy for RRC H 1 meaning
c 3 1175->538, seen twice?
2 TOTL lines -> He 1
for c13 if thor open:
magziarz, 10^23, use 2000 korista and goad abundances apj, also default abundance
2017-03-29 08:46:09 +00:00
use notes from paper to design contour plots
what is the right way to model the components? check mehdipour and magdziarz paper, and comptonization paper
2017-05-02 05:04:17 +00:00
more?
2017-06-17 05:20:37 +00:00
how many collapsed levels do we have?
15 for H⁰ and He⁺, 2 for everything else
other codes:
mappings, ion, X-STAR
print iso collapsed ✓
include lines:
8205A
BAC 3646
BAC 0
Pac 0
hapsed lines
print line cutoff reduced to -- nevermind
