Image de couverture de livre

Reconciling concentration to virial mass relations

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Leier, Dominik, Ferreras, Ignacio, Negri, Andrea, Saha, Prasenjit
Format:	Preprint
Publié:	2024
Sujets:	Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

Gravitational lensing of fast radio bursts: prospects for probing microlens populations in lensing galaxies
par: Meena, Ashish Kumar, et autres
Publié: (2025)

Galaxy cluster virial quantities from extrapolating strong lensing mass profiles
par: Maraboli, Enrico, et autres
Publié: (2025)

Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
par: Sharbaf, Z., et autres
Publié: (2024)

Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
par: Wang, Kai, et autres
Publié: (2025)

Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
par: Shao, Mufan, et autres
Publié: (2023)

Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback
par: Bera, Ankita, et autres
Publié: (2025)

Dark Matter Particle Flux in a Dynamically Self-consistent Milky Way Model
par: Stanic, Lucijana, et autres
Publié: (2025)

Discovery of a >13 Mpc long X-ray filament between two galaxy clusters beyond three times their virial radii
par: Dietl, J., et autres
Publié: (2024)

Too many protoclusters? Reconciling the overabundance of cluster progenitors within the first billion years of the Universe
par: Witten, Callum, et autres
Publié: (2026)

Establishing HI mass v.s. stellar mass and halo mass scaling relations using an abundance matching method
par: Lu, Yi, et autres
Publié: (2024)

DINGO/GAMA /WAVES: HI-halo mass relation
par: Dev, Ajay, et autres
Publié: (2026)

Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
par: Wang, Kai, et autres
Publié: (2024)

MIGHTEE-HI: The HI mass-stellar mass relation of massive galaxies and the HI mass function at 0.25<z<0.5
par: Pan, Hengxing, et autres
Publié: (2025)

MIGHTEE-HI: The radial acceleration relation with resolved stellar mass measurements
par: Vărăşteanu, Andreea A., et autres
Publié: (2025)

Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
par: Chen, Mingjing, et autres
Publié: (2024)

The origin of scatter in the X-ray luminosity - halo mass relation of galaxy clusters
par: Braspenning, Joey, et autres
Publié: (2025)

Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
par: Li, Shun-Sheng, et autres
Publié: (2024)

Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
par: Oyarzún, Grecco A., et autres
Publié: (2024)

Probing the co-evolution of SMBHs and their hosts from scaling relations pairwise residuals: dominance of stellar velocity dispersion and host halo mass
par: Shankar, Francesco, et autres
Publié: (2025)

The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
par: Pallottini, A., et autres
Publié: (2024)

The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies
par: Júlio, Mariana P., et autres
Publié: (2025)

Do Unusually Cold Starburst Galaxies Exist? A Case Study
par: Riechers, Dominik A.
Publié: (2024)

Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
par: Jun, Rui Lan, et autres
Publié: (2025)

An almost dark galaxy with the mass of the Small Magellanic Cloud
par: Montes, Mireia, et autres
Publié: (2023)

Quantifying the impact of AGN feedback on the large-scale matter distribution using two- and three-point statistics
par: Saha, Bipradeep, et autres
Publié: (2024)

Unveiling the (in)consistencies among the galaxy stellar mass function, star formation histories, satellite abundances and intracluster light from a semi-empirical perspective
par: Fu, Hao, et autres
Publié: (2024)

Studying [CII] Emission in Low-mass Galaxies at z ~ 7
par: Glazer, Kelsey, et autres
Publié: (2023)

Massive star clusters detected by JWST as natural birth places to form intermediate-mass black holes
par: Schleicher, Dominik R. G., et autres
Publié: (2026)

The mass accretion history of dark matter haloes down to Earth mass
par: Liu, Yizhou, et autres
Publié: (2023)

Massive stars as gravitationally lensed transients -- Insights on the high-mass initial mass function
par: Li, Sung Kei
Publié: (2026)

The initial mass function of stars
par: Kroupa, Pavel, et autres
Publié: (2024)

On the relative CNO underabundance in quasar absorption systems at $z \sim 3$ arising from Population III enrichment and attenuation by intermediate-mass black holes and primordial baryon accretion
par: Macedo, Murilo, et autres
Publié: (2026)

The XXL Survey LI. Pressure profile and $Y_{\rm SZ}$-$M$ scaling relation in three low-mass galaxy clusters at $z\sim1$ observed with NIKA2
par: Adam, R., et autres
Publié: (2023)

Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
par: Mountrichas, G., et autres
Publié: (2026)

The accretion of a solar mass per day by a 17-billion solar mass black hole
par: Wolf, Christian, et autres
Publié: (2024)

Wandering intermediate-mass black holes in Milky Way-mass galaxies in cosmological simulations: myth or reality?
par: van Donkelaar, Floor, et autres
Publié: (2024)

The baryon census and the mass-density of stars, neutral gas, and hot gas as a function of halo mass
par: Dev, Ajay, et autres
Publié: (2024)

The influence of baryons on low-mass haloes
par: Zheng, Haonan, et autres
Publié: (2024)

The mass distribution in and around the Local Group
par: Wempe, Ewoud, et autres
Publié: (2026)

JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at $z=0.4$
par: Diego, Jose M., et autres
Publié: (2023)