21cmEMU: an emulator of 21cmFAST summary observables
Fuente:
arXiv
Guardado en:
| Autores principales: | Breitman, Daniela, Mesinger, Andrei, Murray, Steven, Prelogovic, David, Qin, Yuxiang, Trotta, Roberto |
|---|---|
| Formato: | Preprint |
| Publicado: |
2023
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables
por: Breitman, Daniela, et al.
Publicado: (2026)
por: Breitman, Daniela, et al.
Publicado: (2026)
How informative are summaries of the cosmic 21-cm signal?
por: Prelogović, David, et al.
Publicado: (2024)
por: Prelogović, David, et al.
Publicado: (2024)
The EDGES measurement disfavors an excess radio background during the cosmic dawn
por: Cang, Junsong, et al.
Publicado: (2024)
por: Cang, Junsong, et al.
Publicado: (2024)
Sample Variance Denoising in Cylindrical 21-cm Power Spectra
por: Breitman, Daniela, et al.
Publicado: (2025)
por: Breitman, Daniela, et al.
Publicado: (2025)
21cm signal sensitivity to dark matter decay
por: Facchinetti, Gaétan, et al.
Publicado: (2023)
por: Facchinetti, Gaétan, et al.
Publicado: (2023)
Detecting galaxy-21-cm cross-correlation during reionization
por: Gagnon-Hartman, Samuel, et al.
Publicado: (2025)
por: Gagnon-Hartman, Samuel, et al.
Publicado: (2025)
The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization
por: Nikolić, Ivan, et al.
Publicado: (2024)
por: Nikolić, Ivan, et al.
Publicado: (2024)
An emulator-based forecasting on astrophysics and cosmology with 21 cm and density cross-correlations during EoR
por: Maity, Barun
Publicado: (2025)
por: Maity, Barun
Publicado: (2025)
The 21cm-galaxy cross-correlation: Realistic forecast for 21cm signal detection and reionisation constraints
por: Hutter, Anne, et al.
Publicado: (2025)
por: Hutter, Anne, et al.
Publicado: (2025)
Inferring reionization and galaxy properties from the patchy kinetic Sunyaev-Zel'dovich signal
por: Nikolić, Ivan, et al.
Publicado: (2023)
por: Nikolić, Ivan, et al.
Publicado: (2023)
Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum
por: Ventura, Emanuele M., et al.
Publicado: (2025)
por: Ventura, Emanuele M., et al.
Publicado: (2025)
A covariant formulation for cosmological radiative transfer of the 21-cm line
por: Chan, Jennifer Y. H., et al.
Publicado: (2024)
por: Chan, Jennifer Y. H., et al.
Publicado: (2024)
Exploring the High-Redshift 21-cm Signal via Self-Consistent Simulations using Artificial Neural Network Emulation
por: Feathers, Colton R., et al.
Publicado: (2026)
por: Feathers, Colton R., et al.
Publicado: (2026)
Deep learning approach for identification of HII regions during reionization in 21-cm observations -- II. foreground contamination
por: Bianco, Michele, et al.
Publicado: (2023)
por: Bianco, Michele, et al.
Publicado: (2023)
21-cm fluctuations from primordial magnetic fields
por: Cruz, Hector Afonso G., et al.
Publicado: (2023)
por: Cruz, Hector Afonso G., et al.
Publicado: (2023)
The 21-cm signal during the end stages of reionization
por: Giri, Sambit K., et al.
Publicado: (2024)
por: Giri, Sambit K., et al.
Publicado: (2024)
Mapping reionization bubbles in the JWST era I: empirical edge detection with Lyman alpha emission from galaxies
por: Lu, Ting-Yi, et al.
Publicado: (2024)
por: Lu, Ting-Yi, et al.
Publicado: (2024)
The effect of a short mean free path on HII regions and 21-cm tomography during reionization
por: Wyatt, Michael M., et al.
Publicado: (2025)
por: Wyatt, Michael M., et al.
Publicado: (2025)
Constraining Statistical Isotropy using 21cm Power Spectrum and Bispectrum
por: Joshi, Bhuwan, et al.
Publicado: (2025)
por: Joshi, Bhuwan, et al.
Publicado: (2025)
A Generative Modeling Approach to Reconstructing 21-cm Tomographic Data
por: Sabti, Nashwan, et al.
Publicado: (2024)
por: Sabti, Nashwan, et al.
Publicado: (2024)
Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe
por: Dhandha, Jiten, et al.
Publicado: (2025)
por: Dhandha, Jiten, et al.
Publicado: (2025)
$\texttt{21cmLSTM}$: A Fast Memory-based Emulator of the Global 21 cm Signal with Unprecedented Accuracy
por: Jones, J. Dorigo, et al.
Publicado: (2024)
por: Jones, J. Dorigo, et al.
Publicado: (2024)
Forecasting 21-cm power spectrum sensitivity to dark Matter-baryon scattering
por: Rahimieh, Aryan, et al.
Publicado: (2025)
por: Rahimieh, Aryan, et al.
Publicado: (2025)
Investigating the Reionization Epoch through 21\,cm and Line Intensity Mapping Experiments
por: Roy, Anirban, et al.
Publicado: (2025)
por: Roy, Anirban, et al.
Publicado: (2025)
The relative constraining power of the high-$z$ 21-cm dipole and monopole signals
por: Mirocha, Jordan, et al.
Publicado: (2024)
por: Mirocha, Jordan, et al.
Publicado: (2024)
Exploring the effect of different cosmologies on the Epoch of Reionization 21-cm signal with POLAR
por: Acharya, Anshuman, et al.
Publicado: (2024)
por: Acharya, Anshuman, et al.
Publicado: (2024)
Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history
por: Libanore, Sarah, et al.
Publicado: (2023)
por: Libanore, Sarah, et al.
Publicado: (2023)
Inferring population III star properties from the 21-cm global signal
por: Ukai, Sho, et al.
Publicado: (2026)
por: Ukai, Sho, et al.
Publicado: (2026)
The mass distribution of the first stars can be determined via the 21-cm signal
por: Gessey-Jones, T., et al.
Publicado: (2025)
por: Gessey-Jones, T., et al.
Publicado: (2025)
Predicting the 21 cm field with a Hybrid Effective Field Theory approach
por: Baradaran, Danial, et al.
Publicado: (2024)
por: Baradaran, Danial, et al.
Publicado: (2024)
Narrowing the discovery space of the cosmological 21-cm signal using multi-wavelength constraints
por: Dhandha, Jiten, et al.
Publicado: (2025)
por: Dhandha, Jiten, et al.
Publicado: (2025)
Simulations of the 21cm emission line for upcoming large-scale HI galaxy surveys
por: Mayor, Joël, et al.
Publicado: (2026)
por: Mayor, Joël, et al.
Publicado: (2026)
Cosmic variance suppression in radiation-hydrodynamic modeling of the reionization-era 21-cm signal
por: Acharya, Anshuman, et al.
Publicado: (2023)
por: Acharya, Anshuman, et al.
Publicado: (2023)
Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization
por: Chakraborty, Anirban, et al.
Publicado: (2026)
por: Chakraborty, Anirban, et al.
Publicado: (2026)
Impact of astrophysical scatter on the Epoch of Reionization [H I]$_{\rm 21cm}$ bispectrum
por: Murmu, Chandra Shekhar, et al.
Publicado: (2023)
por: Murmu, Chandra Shekhar, et al.
Publicado: (2023)
Insights into the 21 cm field from the vanishing cross-power spectrum at the epoch of reionization
por: Moriwaki, Kana, et al.
Publicado: (2024)
por: Moriwaki, Kana, et al.
Publicado: (2024)
Impact of astrophysical effects on the dark matter mass constraint with 21cm intensity mapping
por: Murakami, Koya, et al.
Publicado: (2023)
por: Murakami, Koya, et al.
Publicado: (2023)
Mapping reionization bubbles in the JWST era II: inferring the position and characteristic size of individual bubbles
por: Nikolić, Ivan, et al.
Publicado: (2025)
por: Nikolić, Ivan, et al.
Publicado: (2025)
The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars
por: Cruz, Hector Afonso G., et al.
Publicado: (2024)
por: Cruz, Hector Afonso G., 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)
por: Chhabra, Minal, et al.
Publicado: (2025)
Ejemplares similares
-
21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables
por: Breitman, Daniela, et al.
Publicado: (2026) -
How informative are summaries of the cosmic 21-cm signal?
por: Prelogović, David, et al.
Publicado: (2024) -
The EDGES measurement disfavors an excess radio background during the cosmic dawn
por: Cang, Junsong, et al.
Publicado: (2024) -
Sample Variance Denoising in Cylindrical 21-cm Power Spectra
por: Breitman, Daniela, et al.
Publicado: (2025) -
21cm signal sensitivity to dark matter decay
por: Facchinetti, Gaétan, et al.
Publicado: (2023)