Image de couverture de livre

Signatures of Accreting Black Holes in Line Intensity Mapping

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Ogata, Erika, Moriwaki, Kana, Lidz, Adam, Jun, Rui Lan, Yoshida, Naoki
Format:	Preprint
Publié:	2026
Sujets:	Astrophysics of Galaxies
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
par: Moriwaki, Kana, et autres
Publié: (2025)

Insights into the 21 cm field from the vanishing cross-power spectrum at the epoch of reionization
par: Moriwaki, Kana, et autres
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)

The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
par: Jun, Rui Lan, et autres
Publié: (2024)

Line-Intensity Mapping
par: Chang, Tzu-Ching, et autres
Publié: (2026)

Signatures of high-redshift galactic outflows in the thermal Sunyaev Zel'dovich effect
par: Sun, Guochao, et autres
Publié: (2024)

HOLESOM: Constraining the Properties of Slowly-Accreting Massive Black Holes with Self-Organizing Maps
par: La Torre, Valentina, et autres
Publié: (2024)

LIMFAST. IV. Learning High-Redshift Galaxy Formation from Multiline Intensity Mapping with Implicit Likelihood Inference
par: Sun, Guochao, et autres
Publié: (2025)

Studying the Dust Distribution Around Accreting Black Holes with Reverberation Mapping Using PRIMA
par: Gorjian, Varoujan, et autres
Publié: (2025)

Trinity VII. Predictions for the Observable Correlation Functions of Accreting Black Holes
par: Knox, Oddisey, et autres
Publié: (2025)

An Accreting Supermassive Black Hole Buried in a Faint Dwarf Galaxy
par: Paswan, Abhishek, et autres
Publié: (2024)

The Origins of Gas Accreted by Supermassive Black Holes: the Importance of Recycled Gas
par: Choi, Ena, et autres
Publié: (2023)

Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities
par: Cleri, Nikko J., et autres
Publié: (2025)

Migration of Accreting Planets and Black Holes in Disks
par: Laune, JT, et autres
Publié: (2024)

Semi-Empirical Approach to [CII] Line Intensity Mapping
par: Roy, Anirban, et autres
Publié: (2024)

Effects of Bursty Star Formation on [CII] Line Intensity Mapping of High-redshift Galaxies
par: Liu, Lun-Jun, et autres
Publié: (2024)

Three-Dimensional Stacking as a Line Intensity Mapping Statistic
par: Dunne, D. A., et autres
Publié: (2025)

Tracing Large-Scale Structure Morphology with Multiwavelength Line Intensity Maps
par: Dosibhatla, Manas Mohit, et autres
Publié: (2025)

Reionization Bubbles from Real-Space Cross Correlations of Line Intensity Maps
par: Thélie, Emilie, et autres
Publié: (2026)

Investigating the Reionization Epoch through 21\,cm and Line Intensity Mapping Experiments
par: Roy, Anirban, et autres
Publié: (2025)

Cross-correlation Techniques to Mitigate the Interloper Contamination for Line Intensity Mapping Experiments
par: Roy, Anirban, et autres
Publié: (2023)

Fuzzy Dark Matter Constraints from the Hubble Frontier Fields
par: Sipple, Jackson, et autres
Publié: (2024)

The Millimeter/X-ray Relation in Rapidly Accreting Supermassive Black Holes at z <0.16
par: Venselaar, Sophie M., et autres
Publié: (2026)

Widespread Extended [CII] Emission in High-Redshift Galaxies: Insights from the FIRE-2 Cosmological Zoom-in Simulations
par: Liu, Lun-Jun, et autres
Publié: (2026)

Detecting the Black Hole Candidate Population in M51's Young Massive Star Clusters: Constraints on Accreting Intermediate Mass Black Holes
par: Dage, Kristen C., et autres
Publié: (2024)

The X-ray Emission of NGC 5005: An Unobscured Low-Luminosity AGN with a Weakly Accreting Broad-Line Region
par: Falcão, Anna Trindade, et autres
Publié: (2025)

A New Framework for ISM Emission Line Models: Connecting Multi-Scale Simulations Across Cosmological Volumes
par: Yang, Shengqi, et autres
Publié: (2024)

Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XV. Reverberation Mapping of Mg II Emission Lines
par: Bai, Hua-Rui, et autres
Publié: (2025)

Early Structure Formation from Primordial Density Fluctuations with a Blue, Tilted Power Spectrum: High-Redshift Galaxies
par: Hirano, Shingo, et autres
Publié: (2023)

NGC 3259: A Signal for an Untapped Population of Slowly Accreting Intermediate-Mass Black Holes
par: Grishin, Kirill A., et autres
Publié: (2025)

Continuum Reverberation Mapping of Accretion Disks Surrounding Supermassive Black Hole Binaries: Observational Signatures
par: Fu, Yi-Xin, et autres
Publié: (2025)

The relative constraining power of the high-$z$ 21-cm dipole and monopole signals
par: Mirocha, Jordan, et autres
Publié: (2024)

A Comprehensive JWST/NIRSpec Census of Broad-Line Active Galactic Nuclei: Faint, Tiny, but Highly Accreting Sources in the Remote Universe
par: Baccus, Caroline, et autres
Publié: (2025)

Forecasts and Statistical Insights for Line Intensity Mapping Cross-Correlations: A Case Study with 21cm x [CII]
par: Fronenberg, Hannah, et autres
Publié: (2024)

Bayesian Multi-line Intensity Mapping
par: Cheng, Yun-Ting, et autres
Publié: (2024)

Do cosmological simulations reproduce the [OIII] 88 $μ$m line emission and properties of JWST-discovered galaxies at $z \geq 12$?
par: Yang, Shengqi, et autres
Publié: (2025)

Analytical strong line diagnostics and their redshift evolution
par: Yang, Shengqi, et autres
Publié: (2023)

A merger-driven scenario for clumpy galaxy formation in the epoch of reionization: Physical properties of clumps in the FirstLight simulation
par: Nakazato, Yurina, et autres
Publié: (2024)

The SDSS-V Black Hole Mapper Reverberation Mapping Project: Light Echoes of the Coronal Line Region in a Luminous Quasar
par: Smith, Theodore B., et autres
Publié: (2025)

Disentangling Target Lines from Interlopers and Continuum with Neural Networks: A SPHEREx Intensity Mapping Case Study
par: Cagliari, Marina S., et autres
Publié: (2025)