cloudy-agn/notes

immediate things
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trim labels in fort file header, do any other header things
look at paper from kirk's student and find the value of that parameter
copy grids from thor


this shows only the transition between 1s and 2p... where are the rest of the contributions?

if indeed cloudy is meaning to print these out individually?

this may not be true for hydrogen-like iron, but for H-alpha the three transitions should be included

is this just sloppy notation in output file, or is this really accurate and then where is all the rest of it?




save species line "species_lines" all
save species labels "species_labels" all


OR

save species labels "species_labels"
H[:]
end 


For SED
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At low end transition to slope of 2

at high end cutoff to slope -2.5

check out Kirk's slope explanation for better approximations



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




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?

        



    ✓   faint to equivalent width of 0.001 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

    ✓   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



    check on ratios of inwd lines for blends 

    check hazy for RRC H  1 meaning

    c  3  1175->538, seen twice? -- looked again, I don't see that now

    2 TOTL lines -> He 1   

    for c13 if thor open:

        magziarz, 10^23, use 2000 korista and goad abundances apj, also default abundance 



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


    other codes
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    mappings, ion, X-STAR


include lines:

8205A

hapsed lines

BAC 3646 ✓

BAC 0 ✓

Pac 0 ✓



lines not found:

TOTL 1.08299m
He 1 1.08291m # 1S1 to 3P0 <
He 1 1.08303m # 1S1 to 3P1 <
He 1 1.08303m # 1S1 to 3P2
He 1 3888.63A

Ca2K      3934.00A
Ca2H      3969.00A
Ca2X      8498.00A
Ca2Y      8542.00A
Ca2Z      8662.00A



Fe 2      1500.00A
Fe 2      1.15000m
Fe 2      2500.00A
Fe 2      2300.00A
Fe 2      8900.00A
Fe 2      1786.00A
Fe 3      1125.79A


Missing blend for Ne 5  ~1142A

No good matches for these, included closest ones

    Si 2      1813.99A
    Si 2      1531.00A
    Si 2      1307.66A
    Si 2      1263.32A
    Si 3      1207.00A