:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Kang, Jiangang, Zhang, Tong-Jie, He, Peng, Zhu, Ming
Formato:	Preprint
Publicado:	2025
Materias:	Cosmology and Nongalactic Astrophysics
Acceso en línea:	https://arxiv.org/abs/2501.15117
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Estimating constraints on cosmological parameters via the canonical and the differential redshift drift with SKA HI 21-cm observations
por: Kang, Jiangang, et al.
Publicado: (2025)

Toward a direct measurement of the cosmic acceleration: The pilot observation of H I 21cm absorption line at FAST
por: Kang, Jiangang, et al.
Publicado: (2023)

Redshift-space 21-cm bispectrum multipoles as an SKA-era gravity test in the post-reionization Universe
por: Pal, Sourav, et al.
Publicado: (2026)

Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics. Part II. Impact of the realistic foreground and instrumental noise on synthetic SKA1-Low observations
por: Pal, Samit Kumar, et al.
Publicado: (2025)

Post-reionization HI 21-cm signal: A probe of negative cosmological constant
por: Dash, Chandrachud B. V., et al.
Publicado: (2023)

Probing ionized bubbles around luminous sources during reionization with SKA 21-cm observations
por: Mishra, Arnab, et al.
Publicado: (2026)

Sensitivity toward dark matter annihilation imprints on 21-cm signal with SKA-Low: A convolutional neural network approach
por: Natwariya, Pravin Kumar, et al.
Publicado: (2025)

Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics III: Impact of the lightcone effect
por: Potluri, Hemanth, et al.
Publicado: (2026)

Primordial Magnetic Fields at Cosmic Dawn: 21-cm Forecasts with HERA and SKA
por: Worku, Keduse, et al.
Publicado: (2026)

Reconstructing a non-linear interaction in the dark sector with cosmological observations
por: Kang, Jiangang
Publicado: (2021)

Detecting ionized bubbles around luminous sources during the reionization era using HI 21-cm signal
por: Mishra, Arnab, et al.
Publicado: (2024)

Gravitational lensing of 21 cm HI signal: detection prospects at z ~ 1 with uGMRT in galaxy cluster lenses
por: Bharti, Sauraj, et al.
Publicado: (2025)

Probing Reionization up to the Mark: The Marked Power Spectrum to unveil the HI 21-cm signal from the EoR
por: Pandya, Vishrut, et al.
Publicado: (2026)

Cross-Comparison of Galaxies Detected in the CSST Spectroscopic Survey and the SKA HI Survey
por: Liu, Yingfeng, et al.
Publicado: (2026)

Redshift-binned constraints on the Hubble constant under $Λ$CDM, CPL, and Padé cosmography
por: Mo, Zhi-Yuan, et al.
Publicado: (2026)

Impact of Calibration and Position Errors on Astrophysical Parameters of the HI 21cm Signal
por: Tripathi, Anshuman, et al.
Publicado: (2025)

Detectability of the 21 cm signal with BINGO through cross-correlation with photometric surveys
por: Silva, Gabriel A. S., et al.
Publicado: (2025)

Uncovering the Effects of Array Mutual Coupling in 21-cm Experiments with the SKA-Low Radio Telescope
por: O'Hara, Oscar S. D., et al.
Publicado: (2024)

Understanding spectral artefacts in SKA-LOW 21-cm cosmology experiments: the impact of cable reflections
por: O'Hara, Oscar Sage David, et al.
Publicado: (2024)

FLRW Kinematic-Induced Measurement of the Hubble Constant from Cosmic Chronometer and Redshift Drift Observations
por: Jiao, Kang, et al.
Publicado: (2025)

21cmFirstCLASS II. Early linear fluctuations of the 21cm signal
por: Flitter, Jordan, et al.
Publicado: (2023)

Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys
por: Song, Yanling, et al.
Publicado: (2026)

The Impact of Foregrounds on Dark Ages Measurements with the Highly Redshifted 21 cm Line
por: Pober, Jonathan C., et al.
Publicado: (2025)

Exploring HI Galaxy Redshift Survey Strategies for the FAST Core Array Interferometry
por: Li, Zhenglong, et al.
Publicado: (2025)

Exploring the effect of different cosmologies on the Epoch of Reionization 21-cm signal with POLAR
por: Acharya, Anshuman, et al.
Publicado: (2024)

Simulations of the 21cm emission line for upcoming large-scale HI galaxy surveys
por: Mayor, Joël, et al.
Publicado: (2026)

Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions
por: Gkogkou, Athanasia, et al.
Publicado: (2025)

The Signature of Strong High-Redshift Radio Backgrounds on the Cosmic Dawn 21-cm Bispectrum
por: Sikder, Sudipta, et al.
Publicado: (2026)

FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
por: Liu, Diyang, et al.
Publicado: (2024)

Probing the HI distribution at small scales using 21-cm Intensity Mapping at large scales
por: Chhabra, Minal, et al.
Publicado: (2025)

The 21cm-galaxy cross-correlation: Realistic forecast for 21cm signal detection and reionisation constraints
por: Hutter, Anne, et al.
Publicado: (2025)

Probing Decaying Dark Matter Using the Post-EoR HI 21-cm signal
por: Yadav, Mohit, et al.
Publicado: (2024)

The 21-cm signal during the end stages of reionization
por: Giri, Sambit K., et al.
Publicado: (2024)

How informative are summaries of the cosmic 21-cm signal?
por: Prelogović, David, et al.
Publicado: (2024)

Nonlinear reconstruction of 21cm global signal from 21cm power spectrum with artificial neural networks
por: Shimabukuro, Hayato
Publicado: (2024)

Cosmological super-resolution of the 21-cm signal
por: Pochinda, Simon, et al.
Publicado: (2025)

FAST drift scan survey for HI intensity mapping: simulation on Bayesian-stacking-based HI mass function estimation
por: Wang, Jiaxin, et al.
Publicado: (2025)

The morphology of the redshifted 21-cm signal from the Cosmic Dawn
por: Ghara, Raghunath, et al.
Publicado: (2023)

Effect of Primordial Black Holes on the global 21-cm signal
por: Chatterjee, Atrideb
Publicado: (2026)

Ionospheric effect on the synthetic Epoch of Reionization observations with the SKA1-Low
por: Pal, Samit Kumar, et al.
Publicado: (2024)