mirror of
https://asciireactor.com/otho/cloudy-agn.git
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153 lines
3.1 KiB
Plaintext
153 lines
3.1 KiB
Plaintext
immediate things
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trim labels in fort file header, do any other header things
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look at paper from kirk's student and find the value of that parameter
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copy grids from thor
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this shows only the transition between 1s and 2p... where are the rest of the contributions?
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if indeed cloudy is meaning to print these out individually?
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this may not be true for hydrogen-like iron, but for H-alpha the three transitions should be included
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is this just sloppy notation in output file, or is this really accurate and then where is all the rest of it?
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save species line "species_lines" all
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save species labels "species_labels" all
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OR
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save species labels "species_labels"
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H[:]
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end
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2017 grids needed
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mehdipour SED, solar, 10²² - 10²⁴
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magdziarz SED, solar, 10²² - 10²⁴
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magdziarz SED, metals 0.5 & element scale factor carbon 2, 10²² - 10²⁴
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By end of March: two grids run, continuum points decided upon, models decided upon
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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?
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✓ faint to equivalent width of 0.001 angstrom
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✓ compare between c13 and c17 -- show diferences in emergent line lists
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✓ new print lines to help reduce number of printed lines -- and to show old lines?
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✓ run models for comparising: 10.5,19.5
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✓ Why so many Fe 2 lines?
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✓ check if blnds are sums of the expected multiplets
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✓ add in more levels to the H atom, unresolved, 20, also add some to paschen, maybe others -- check how much time is lost
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✓ punch the paschen and balmer lines up to 18
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✓ Read Intrinsic Lines
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□ Smoothing algorithm using n-dimensional smoothing
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□ Contour plots
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✓ Run Grids in c17
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✓ Email about order of lines
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✓ Find blend correlated names and update
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check on ratios of inwd lines for blends
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check hazy for RRC H 1 meaning
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c 3 1175->538, seen twice? -- looked again, I don't see that now
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2 TOTL lines -> He 1
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for c13 if thor open:
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magziarz, 10^23, use 2000 korista and goad abundances apj, also default abundance
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use notes from paper to design contour plots
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what is the right way to model the components? check mehdipour and magdziarz paper, and comptonization paper
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other codes
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mappings, ion, X-STAR
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include lines:
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8205A
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hapsed lines
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BAC 3646 ✓
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BAC 0 ✓
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Pac 0 ✓
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lines not found:
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TOTL 1.08299m
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He 1 1.08291m # 1S1 to 3P0 <
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He 1 1.08303m # 1S1 to 3P1 <
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He 1 1.08303m # 1S1 to 3P2
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He 1 3888.63A
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Ca2K 3934.00A
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Ca2H 3969.00A
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Ca2X 8498.00A
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Ca2Y 8542.00A
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Ca2Z 8662.00A
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Fe 2 1500.00A
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Fe 2 1.15000m
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Fe 2 2500.00A
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Fe 2 2300.00A
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Fe 2 8900.00A
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Fe 2 1786.00A
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Fe 3 1125.79A
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Missing blend for Ne 5 ~1142A
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No good matches for these, included closest ones
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Si 2 1813.99A
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Si 2 1531.00A
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Si 2 1307.66A
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Si 2 1263.32A
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Si 3 1207.00A |