Snaith, O.

In Disguise or Out of Reach: First Clues about In Situ and Accreted Stars in the Stellar Halo of the Milky Way from Gaia DR2

Haywood, M., Di Matteo, P., Lehnert, M. D., Snaith, O., Khoperskov, S., & Gómez, A. (2018) · The Astrophysical Journal

Stellar, planetary, and galactic studiesGalaxies: Formation, Evolution, Phenomena

Cited by 360

Gaia Data Release 3: Properties and validation of the radial velocities

Katz, D., Sartoretti, P., Guerrier, A., Panuzzo, P., Seabroke, G. M., Thévenin, F., Cropper, M., Benson, K., Blomme, R., Haigron, R., et al. (2023) · Astronomy & Astrophysics

Stellar, planetary, and galactic studiesAstronomy and Astrophysical Research

Cited by 351

The Milky Way has no in-situ halo other than the heated thick disc: Composition of the stellar halo and age-dating the last significant merger with Gaia DR2 and APOGEE

Di Matteo, P., Haywood, M., Lehnert, M. D., Katz, D., Khoperskov, S., Snaith, O. N., Gómez, A., & Robichon, N. (2019) · Astronomy & Astrophysics

Stellar, planetary, and galactic studiesGalaxies: Formation, Evolution, Phenomena

Cited by 222

THE DOMINANT EPOCH OF STAR FORMATION IN THE MILKY WAY FORMED THE THICK DISK

Snaith, O. N., Haywood, M., Di Matteo, P., Lehnert, M. D., Combes, F., Katz, D., & Gómez, A. (2014) · The Astrophysical Journal

Stellar, planetary, and galactic studiesGalaxies: Formation, Evolution, Phenomena

Cited by 153