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| [LRK2022] 64 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST19:20:56 |
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trying to find the most relevant references on this object.
More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
2022A&A...665A..57L 
|
17 | D | 1 | 6323 | 23 | Substructure in the stellar halo near the Sun. I. Data-driven clustering in integrals-of-motion space. | LOVDAL S.S., RUIZ-LARA T., KOPPELMAN H.H., et al. | ||
|
2022A&A...665A..58R
|
17 | D | 1 | 74 | 19 | Substructure in the stellar halo near the Sun. II. Characterisation of independent structures. | RUIZ-LARA T., MATSUNO T., LOVDAL S.S., et al. | ||
|
2023A&A...670L...2D
|
90 | X | 2 | 5 | 15 | Gaia DR3 view of dynamical substructure in the stellar halo near the Sun. | DODD E., CALLINGHAM T.M., HELMI A., et al. | ||
| 2024A&A...688A.147F | 45 | X | 1 | 20 | ~ | A determination of the Large Magellanic Cloud dark matter subhalo mass using the Milky Way halo stars in its gravitational wake. | FUSHIMI K.J., MOSQUERA M.E. and DOMINGUEZ M. | ||
| 2024A&A...690A..98C | 134 | X | 3 | 13 | ~ | Filling in the blanks A method to infer the substructure membership and dynamics of 5D stars. | CALLINGHAM T.M. and HELMI A. | ||
| 2025ApJ...983...65Y | 373 | S X | 7 | 16 | ~ | Jormungandr: A Large Substructure Circling the Milky Way Identified from Gaia DR3 Data. | YE X., ZHAO G., ALLENDE PRIETO C., et al. | ||
|
2025A&A...700A.154D
|
140 | X | 3 | 55 | ~ | Chemical characterisation of small substructures in the local stellar halo. | DODD E., MATSUNO T., HELMI A., et al. | ||
| 2025A&A...704A..40T | 140 | X | 3 | 24 | ~ | How well can we unravel the accreted constituents of the Milky Way stellar halo?: A test on cosmological hydrodynamical simulations. | THOMAS G.F., BATTAGLIA G., GRAND R.J.J., et al. | ||
|
2025A&A...704A.180C
|
47 | X | 1 | 6 | ~ | A Walk on the Retrograde Side (WRS) project II. Chemistry to disentangle in situ and accreted components in Thamnos. | CECCARELLI E., MASSARI D., PALLA M., et al. | ||
|
2026A&A...706A.130D
|
100 | X | 2 | 180 | ~ | Globular clusters in ORBIT: Complete dynamical characterisation of the Milky Way globular cluster population through updated orbital reconstruction. | DE LEO M., ZOCCALI M., OLIVARES-CARVAJAL J., et al. |
