LIMFAST. V. Probing Reionization with the Synergy Between 21 cm and Photometric Galaxy Surveys
astro-ph.CO, astro-ph.GA
Submitted: 2026-09-28
Updated: 2026-09-28
Terminology
Sources
- Modeling Cosmic Reionization
- 21-cm cosmology
- Exploring the cosmic dawn and epoch of reionization with 21cm line
- Galaxy Formation and Reionization: Key Unknowns and Expected Breakthroughs by the James Webb Space Telescope
- Probing Reionization with the 21 cm-Galaxy Cross Power Spectrum
- Cross-correlation of the cosmic 21-cm signal and Lyman Alpha Emitters during reionization
- Detectability of 21cm-signal during the Epoch of Reionization with 21cm-Lyman-$\alpha$ emitter cross-correlation. I
- Prospects for 21cm-Galaxy Cross-Correlations with HERA and the Roman High-Latitude Survey
- Insights into the 21 cm field from the vanishing cross-power spectrum at the epoch of reionization
- Detecting galaxy-21-cm cross-correlation during reionization
- The 21cm-galaxy cross-correlation: Realistic forecast for 21cm signal detection and reionisation constraints
- Ly$\alpha$ at Cosmic Dawn with a Simulated Roman Grism Deep Field
- From Grism to IFU: Revising the Redshift and Nature of the Massive Dusty Galaxy S1 with JWST and ALMA
- A cross-bispectrum estimator for CMB-HI intensity mapping correlations
- 3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope
- Clustering redshifts with the 21cm-galaxy cross-bispectrum
- Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
- LIMFAST. III. Timing Cosmic Reionization with the 21 cm and Near-Infrared Backgrounds
- Prospects for ${\rm kSZ^2}$-${\rm 21cm^2}$ Cross-Correlations during Reionization
- Squared-field cross-correlation between kinetic Sunyaev-Zel'dovich effect and 21-cm intensity mapping
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