nearly fully fleshed out now
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@@ -21,7 +21,12 @@
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#pause
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],
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[
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...
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$->$ inaccurate when applied to all halos
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$->$ #text(weight: "bold")[inconsistent] with the N-body output
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#pause
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$->$ stochasticity for a more realistic description?
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]
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)
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@@ -31,13 +36,41 @@
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#image_cell(notebook, cell_id: "profile_plot_alpha_dependence")
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$M_"h" = 6.08 dot 10^11 M_dot.circle$ (fixed)
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$==>$ correction up to $times 5$
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// COMMENTS
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// That will be directly affect the global signal as well
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// shifting
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//
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// Yu-Siu already investigated the more nuanced effect of stochasticity but the approach we propose should supersede that
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#pagebreak()
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== Inferring growth from #smallcaps[Thesan] data
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#lorem(50)
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- already includes precomputed merger trees @Springel2005
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// ideal for rapid iterations
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- follow main progenitor branch back in time
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- fit the exponential model to main progrenitor branch
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// in a parallelized fashion => want to stay fast
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// fix the original mass for max. consistency
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// fix the allowed dynamic range
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- use *individual growth* to select profile
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// this sort of "breaks the degeneracy" between halos of the same mass but different growth histories
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- *self-consistent*#pause$*$#meanwhile treatment of halo growth leveraging the snapshots
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#pagebreak()
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#let notebook = json("../workdir/11_visualization/show_trees.ipynb")
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#[
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#set image(width: 100%, fit: "contain")
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#image_cell(notebook, cell_id: "merger_tree_and_fitting")
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]
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// COMMENTS:
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// no clear trend between mass and growth rate
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