The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
Fuente:
arXiv
Enregistré dans:
| Auteurs principaux: | Jun, Rui Lan, Theuns, Tom, Moriwaki, Kana, Bose, Sownak |
|---|---|
| Format: | Preprint |
| Publié: |
2024
|
| Sujets: | |
| Accès en ligne: | |
| Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
Documents similaires
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)
par: Jun, Rui Lan, et autres
Publié: (2025)
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)
par: Saha, Bipradeep, et autres
Publié: (2024)
Insights into the 21 cm field from the vanishing cross-power spectrum at the epoch of reionization
par: Moriwaki, Kana, et autres
Publié: (2024)
par: Moriwaki, Kana, et autres
Publié: (2024)
CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
par: Moriwaki, Kana, et autres
Publié: (2025)
par: Moriwaki, Kana, et autres
Publié: (2025)
Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
par: Marcuzzo, Elena, et autres
Publié: (2025)
par: Marcuzzo, Elena, et autres
Publié: (2025)
The impact of feedback on the evolution of gas density profiles from galaxies to clusters: a universal fitting formula from the Simba suite of simulations
par: Sorini, Daniele, et autres
Publié: (2024)
par: Sorini, Daniele, et autres
Publié: (2024)
Measurements of the HI intensity mapping power spectrum at low redshifts with MIGHTEE data: comparison with detected HI galaxies
par: Townsend, Junaid, et autres
Publié: (2026)
par: Townsend, Junaid, et autres
Publié: (2026)
Simulations of the accreted stellar halos of low-mass field galaxies
par: Cooper, Andrew P., et autres
Publié: (2025)
par: Cooper, Andrew P., et autres
Publié: (2025)
Modelling the expulsion of baryons from haloes from first principles: the role of feedback and of the cosmological constant
par: Veenema, Oscar, et autres
Publié: (2026)
par: Veenema, Oscar, et autres
Publié: (2026)
Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
par: Collier, Michael, et autres
Publié: (2024)
par: Collier, Michael, et autres
Publié: (2024)
Simulating AGN wind feedback with variable feedback efficiencies in idealised disc galaxies
par: Liang, Jinning, et autres
Publié: (2026)
par: Liang, Jinning, et autres
Publié: (2026)
When galaxies burst: enhanced shot-noise for line-intensity mapping in the JWST era
par: Kovetz, Ely D., et autres
Publié: (2026)
par: Kovetz, Ely D., et autres
Publié: (2026)
Milky Way satellite velocities reveal the Dark Matter power spectrum at small scales
par: Esteban, Ivan, et autres
Publié: (2023)
par: Esteban, Ivan, et autres
Publié: (2023)
The origin of lopsided satellite galaxy distribution around isolated systems in MillenniumTNG
par: Liu, Yikai, et autres
Publié: (2024)
par: Liu, Yikai, et autres
Publié: (2024)
Simulations of the 21cm emission line for upcoming large-scale HI galaxy surveys
par: Mayor, Joël, et autres
Publié: (2026)
par: Mayor, Joël, et autres
Publié: (2026)
Fully non-linear simulations of galaxy intrinsic alignments for weak lensing with the MillenniumTNG lightcone
par: Ferlito, Fulvio, et autres
Publié: (2025)
par: Ferlito, Fulvio, et autres
Publié: (2025)
The effect of baryons on the positions and velocities of satellite galaxies in the MTNG simulation
par: Contreras, Sergio, et autres
Publié: (2025)
par: Contreras, Sergio, et autres
Publié: (2025)
The informativeness of [C II] line-intensity mapping as a probe of the H I content and metallicity of galaxies at the end of reionization
par: Horlaville, Patrick, et autres
Publié: (2023)
par: Horlaville, Patrick, et autres
Publié: (2023)
The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations
par: Contreras, Sergio, et autres
Publié: (2026)
par: Contreras, Sergio, et autres
Publié: (2026)
The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
par: Sorini, Daniele, et autres
Publié: (2024)
par: Sorini, Daniele, et autres
Publié: (2024)
A comparison of pre-existing $Λ$CDM predictions with the abundance of {\it JWST} galaxies at high redshift
par: Lu, Shengdong, et autres
Publié: (2024)
par: Lu, Shengdong, et autres
Publié: (2024)
CONCERTO: Extracting the power spectrum of the [C II ] emission line
par: Van Cuyck, M., et autres
Publié: (2023)
par: Van Cuyck, M., et autres
Publié: (2023)
Probing the Epoch of Reionization using synergies of line intensity mapping
par: Murmu, Chandra Shekhar, et autres
Publié: (2022)
par: Murmu, Chandra Shekhar, et autres
Publié: (2022)
Examining Lyman-alpha Emitters through MillenniumTNG in anticipation of DESI-II
par: Ravi, Jyotsna, et autres
Publié: (2024)
par: Ravi, Jyotsna, et autres
Publié: (2024)
LYRA ultra-faints: The emergence of faint dwarf galaxies in the presence of an early Lyman-Werner background
par: Brown, Shaun T., et autres
Publié: (2025)
par: Brown, Shaun T., et autres
Publié: (2025)
Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone
par: Shen, Delon, et autres
Publié: (2025)
par: Shen, Delon, et autres
Publié: (2025)
Estimation of line-of-sight velocities of individual galaxies using neural networks I. Modelling redshift-space distortions at large scales
par: Chen, Hongxiang, et autres
Publié: (2023)
par: Chen, Hongxiang, et autres
Publié: (2023)
Central galaxy alignments. Dependence on the mass and the large-scale environment
par: Rodriguez, Facundo, et autres
Publié: (2025)
par: Rodriguez, Facundo, et autres
Publié: (2025)
Unveiling the small-scale web around galaxies with miniJPAS and DESI
par: Galárraga-Espinosa, Daniela, et autres
Publié: (2025)
par: Galárraga-Espinosa, Daniela, et autres
Publié: (2025)
The case for large-scale AGN feedback in galaxy formation simulations: insights from XFABLE
par: Bigwood, Leah, et autres
Publié: (2025)
par: Bigwood, Leah, et autres
Publié: (2025)
Probing the HI distribution at small scales using 21-cm Intensity Mapping at large scales
par: Chhabra, Minal, et autres
Publié: (2025)
par: Chhabra, Minal, et autres
Publié: (2025)
Exploring the signature of assembly bias and modified gravity using small-scale clusterings of galaxies
par: Wang, Yirong, et autres
Publié: (2025)
par: Wang, Yirong, et autres
Publié: (2025)
Large-scale excess HI absorption around $z\approx4$ galaxies detected in a background galaxy spectrum in the MUSE eXtremely Deep Field
par: Matthee, Jorryt, et autres
Publié: (2023)
par: Matthee, Jorryt, et autres
Publié: (2023)
ELG$\times$LRG distribution through dark matter halo dynamics
par: Favole, Ginevra, et autres
Publié: (2025)
par: Favole, Ginevra, et autres
Publié: (2025)
Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
par: Galbiati, M., et autres
Publié: (2024)
par: Galbiati, M., et autres
Publié: (2024)
Momentum power spectrum of SDSS galaxies by massE cosmic ruler: 2.1x improvement in measure of growth rate
par: Shi, Yong, et autres
Publié: (2024)
par: Shi, Yong, et autres
Publié: (2024)
The abundance of dark matter haloes down to Earth mass
par: Zheng, Haonan, et autres
Publié: (2023)
par: Zheng, Haonan, et autres
Publié: (2023)
MIGHTEE-HI: HI galaxy properties in the large scale structure environment at z~0.37 from a stacking experiment
par: Sinigaglia, Francesco, et autres
Publié: (2024)
par: Sinigaglia, Francesco, et autres
Publié: (2024)
The SAMI Galaxy Survey: large-scale environment affects galaxy spin amplitudes and the formation of slow rotators
par: Barsanti, Stefania, et autres
Publié: (2025)
par: Barsanti, Stefania, et autres
Publié: (2025)
CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
par: Gu, Yizhou, et autres
Publié: (2024)
par: Gu, Yizhou, et autres
Publié: (2024)
Documents similaires
-
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) -
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) -
Insights into the 21 cm field from the vanishing cross-power spectrum at the epoch of reionization
par: Moriwaki, Kana, et autres
Publié: (2024) -
CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
par: Moriwaki, Kana, et autres
Publié: (2025) -
Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
par: Marcuzzo, Elena, et autres
Publié: (2025)