Table 4
Literature results for the logarithm inner slope of the DM halo of Sculptor.
2-pop | Method | Dataset | Anisotropy | Data | γ flex | Result | |
---|---|---|---|---|---|---|---|
B08 | YES | Jeans | B08 | OM rad(r) | Binned | NO | Both fit, core preferred |
W11 | YES | Estimator | W09 | constant | Discrete | - | ![]() |
AE12 | YES | DF | B08 | rad(r) | Binned | NO | Both fit, core preferred |
B13a | NO | Schwar. | W09 & B08 | Free | Binned | YES | Unconstrained |
B13b | NO | Schwar. | W09 & B08 | Free | Binned | NO | Unconstrained |
R14 | NO | Schwar. | W09 | Free | Discrete | YES | Unconstrained |
Z16 | YES | Axi. Jeans | W09 | Constant | Discrete | YES | γ=0.5 ± 0.3 |
S17 | YES | DF | W09/B08 | Tang/Rad (r) | Binned | NO | Depends on dataset |
K19 | NO | Jeans | W09 | Free | Binned | NO | Both fit core preferred |
R19 | NO | Jeans | W09 | Free | Binned | YES | ![]() |
H20 | NO | Axi. Jeans | W09 | Constant | Binned | YES | ![]() |
P20 | NO | DF | I19 | Free | Binned | NO | Core |
E23 | NO | M.L. | W09 | - | Discrete | - | Cusp |
This work | YES | DF | T23 | Free | Discrete | YES | ![]() |
Notes. Column 1 lists the literature works. Column 2 indicates whether the authors use a two-population model or assume that all the stars belong a single population. Column 3 lists the mass modeling method used, M.L. stands for machine learning. Column 4 shows the dataset the authors used and indicates whether the datasets were combined (W09 & B08) or each one was used independently (W09/B08). Column 5 lists the assumpsion made on the anisotropy profile, “OM” stands for “Osipkov-Merritt” profile (Osipkov 1979; Merritt 1985), and rad and tang for only radial or only tangential orbits. Column 6 indicates whether the analysis is done on the bases of binned data or discrete data. Column 7 indicates whether the value assume for γ in the potential is flexible or whether the authors only tried different cases and compare them. Finally, in Column 8 we list the result of that work.
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