Imagen de Portada

The structure of the stellar halo of the Andromeda galaxy explored with the NB515 for Subaru/HSC. I.: New Insights on the stellar halo up to 120 kpc

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Ogami, Itsuki, Tanaka, Mikito, Komiyama, Yutaka, Chiba, Masashi, Guhathakurta, Puragra, Kirby, Evan N., Wyse, Rosemary F. G., Filion, Carrie, Gilbert, Karoline M., Escala, Ivanna, Mori, Masao, Kirihara, Takanobu, Tanaka, Masayuki, Ishigaki, Miho N., Hayashi, Kohei, Lee, Myung Gyoon, Sharma, Sanjib, Kalirai, Jason S., Lupton, Robert H.
Formato:	Preprint
Publicado:	2024
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Simultaneous Formation of the Andromeda Giant Southern Stream and the Substructures in the Andromeda Halo
por: Yamaguchi, Misa, et al.
Publicado: (2025)

Detection of a Spatially Extended Stellar Population in M33: A Shallow Stellar Halo?
por: Ogami, Itsuki, et al.
Publicado: (2024)

Triangulum IV: A Possible Ultra-Diffuse Satellite of M33
por: Ogami, Itsuki, et al.
Publicado: (2024)

Subaru/HSC NB395 view of NGC 5466: metallicity, mass function, and the nature of its tidal stream
por: Ogami, Itsuki, et al.
Publicado: (2026)

Final results for mapping the Milky Way's stellar halo with blue horizontal-branch stars selected from the Subaru Hyper Supreme-Cam Survey
por: Fukushima, Tetsuya, et al.
Publicado: (2024)

Constructing a Pristine View of Extended Globular Cluster Structure
por: Kuzma, Pete B., et al.
Publicado: (2025)

Estimating Fe and Mg Abundances in the Milky Way Dwarf Galaxies Using Subaru/HSC and DEIMOS
por: Hong, Jihye, et al.
Publicado: (2025)

The Extended Stellar Distribution in the Outskirts of the Ursa Minor Dwarf Spheroidal Galaxy
por: Sato, Kyosuke S., et al.
Publicado: (2025)

The Milky Way Tomography with Subaru Hyper Suprime-Cam. II. Global halo structure
por: Suzuki, Yoshihisa, et al.
Publicado: (2026)

Final Results of Search for New Milky Way Satellites in the Hyper Suprime-Cam Subaru Strategic Program Survey: Discovery of Two More Candidates
por: Homma, Daisuke, et al.
Publicado: (2023)

The Star Formation and Chemical Evolution Histories of Ursa Minor Dwarf Spheroidal Galaxy
por: Sato, Kyosuke S., et al.
Publicado: (2025)

Dynamical streams in the local stellar halo
por: Dillamore, Adam M., et al.
Publicado: (2025)

Blind source separation of the stellar halo
por: Davies, Elliot Y., et al.
Publicado: (2024)

Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
por: Luo, Wentao, et al.
Publicado: (2022)

Machine Learning Techniques to Distinguish Giant Stars from Dwarf Stars Using Only Photometry -- Pushing Redwards
por: Ding, Keyi, et al.
Publicado: (2025)

Effectiveness of halo and galaxy properties in reducing the scatter in the stellar-to-halo mass relation
por: Pei, Wenxiang, et al.
Publicado: (2024)

Galaxy Morphologies Revealed with Subaru HSC and Super-Resolution Techniques II: Environmental Dependence of Galaxy Mergers at z~2-5
por: Shibuya, Takatoshi, et al.
Publicado: (2024)

The stellar-to-halo mass relation of central galaxies across three orders of halo mass
por: Toptun, Victoria, et al.
Publicado: (2026)

The response of the inner dark matter halo to stellar bars
por: Marostica, Daniel A., et al.
Publicado: (2024)

Chemical characterisation of small substructures in the local stellar halo
por: Dodd, Emma, et al.
Publicado: (2025)

Characterizing the velocity anisotropy of the Milky Way's stellar halo
por: Barbosa, F. O., et al.
Publicado: (2026)

Search for Brown Dwarfs in IC 1396 with Subaru HSC: Interpreting the Impact of Environmental Factors on Sub-stellar Population
por: Gupta, Saumya, et al.
Publicado: (2024)

Uncovering the Ghostly Remains of an Extremely Diffuse Satellite in the Remote Halo of NGC 253
por: Okamoto, Sakurako, et al.
Publicado: (2024)

The active role of co-evolving haloes in stellar bar formation
por: Frosst, Matthew, et al.
Publicado: (2024)

Accreted stars and stellar haloes of simulated galaxies in TNG50
por: Celiz, Bruno M., et al.
Publicado: (2025)

Probing the dark matter haloes of external galaxies with stellar streams
por: Walder, Madison, et al.
Publicado: (2024)

Unveiling the formation channels of stellar halos through their chemical fingerprints
por: Gonzalez-Jara, Jenny, et al.
Publicado: (2024)

Simulations of the accreted stellar halos of low-mass field galaxies
por: Cooper, Andrew P., et al.
Publicado: (2025)

Searching for ghosts in the galactic halo: what can we learn about the formation of the galaxy from the stellar halo?
por: L. A. Aguilar
Publicado: (2006)

Progenitor diversity in the accreted stellar halos of Milky Way-like galaxies
por: Pu, Sy-Yun, et al.
Publicado: (2024)

Age and metallicity of low-mass galaxies: from their centres to their stellar halos
por: Tau, Elisa A., et al.
Publicado: (2025)

Mapping the anisotropic Galactic stellar halo with Blue Horizontal Branch stars
por: Amarante, João A. S., et al.
Publicado: (2024)

The Sagittarius stellar stream embedded in a fermionic dark matter halo
por: Collazo, Santiago, et al.
Publicado: (2025)

GSE vs. LMC: reshaping of radially biased stellar haloes by satellites
por: Dillamore, Adam M., et al.
Publicado: (2026)

Probing the spatial and velocity anisotropies in stellar halos from the Aquarius simulations
por: Mondal, Amit, et al.
Publicado: (2023)

The stellar bar - dark matter halo connection in the TNG50 simulations
por: Ansar, Sioree, et al.
Publicado: (2023)

Galactic Archaeology with the Subaru `Ōnohi`ula Prime Focus Spectrograph Strategic Program
por: Chiba, Masashi, et al.
Publicado: (2026)

A systematic search for rapid transients in the Subaru HSC-SSP transient survey
por: Toshikage, Seiji, et al.
Publicado: (2024)

The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies
por: Tau, Elisa A., et al.
Publicado: (2024)

Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
por: Wang, Kai, et al.
Publicado: (2025)