| Autor: |
Reino, Stella, Rossi, Elena M, Sanderson, Robyn E, Sellentin, Elena, Helmi, Amina, Koppelman, Helmer H, Sharma, Sanjib |
| Předmět: |
|
| Zdroj: |
Monthly Notices of the Royal Astronomical Society; 5/30/2022, Vol. 512 Issue 3, p4455-4463, 9p |
| Abstrakt: |
Applying the density estimator to the entire distribution as constructed, including both clusters, produces estimates that differ only fractionally from those estimated for each cluster individually (Fig. Using EnLink on this density distribution produces density estimates that are severely sheared for the cluster with fewer points, as shown in the lower left-hand panel of Fig. Keywords: errata; addenda; methods: numerical; Galaxy: fundamental parameters; Galaxy: kinematics and dynamics; Galaxy: structure; dark matter EN errata addenda methods: numerical Galaxy: fundamental parameters Galaxy: kinematics and dynamics Galaxy: structure dark matter 4455 4463 9 04/18/22 20220530 NES 220530 This is an erratum to the paper 'Galactic potential constraints from clustering in action space of combined stellar stream data' (Reino et al. [11]). [Extracted from the article] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
|
