Imagen de Portada

Machine learning analysis of Photometric data from the Dark Energy Survey

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Abdalla, Elcio, Abdalla, Filipe B., Marins, Alessandro, Queiroz, Amilcar, Ribeiro, Rafael M., Souza, Alex S. C.
Formato:	Preprint
Publicado:	2025
Materias:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Investigating cross-correlations between cosmic microwave background lensing and 21 cm intensity mapping
por: Marins, Alessandro, et al.
Publicado: (2025)

Cosmological Remapping for Efficient Generation of 21 cm Intensity Mapping Mocks
por: Mokeddem, Rahima, et al.
Publicado: (2025)

Machine learning based Photometric Redshifts for Galaxies in the North Ecliptic Pole Wide field: catalogs of spectroscopic and photometric redshifts
por: Kim, Taewan, et al.
Publicado: (2025)

WFC3 Infrared Spectroscopic Parallel (WISP) Survey: Photometric and Emission Line Data Release
por: Battisti, A. J., et al.
Publicado: (2024)

Constraints on cosmology and baryonic feedback with joint analysis of Dark Energy Survey Year 3 lensing data and ACT DR6 thermal Sunyaev-Zel'dovich effect observations
por: Pandey, S., 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)

Dark Energy Survey Deep Field photometric redshift performance and training incompleteness assessment
por: Cipriano, L. Toribio San, et al.
Publicado: (2023)

Dark Energy Survey Year 6 Results: Synthetic-source Injection Across the Full Survey Using Balrog
por: Anbajagane, D., et al.
Publicado: (2025)

Interacting Dark Sector field theory with phantom crossing
por: Abdalla, E., et al.
Publicado: (2026)

EMU: Cross-correlating EMU Pilot Survey 1 with Dark Energy Survey to constrain the radio galaxy redshift distribution
por: Saraf, Chandra Shekhar, et al.
Publicado: (2025)

Photometric Redshift PDFs via Neural Network Classification for DESI Legacy Imaging Surveys and Pan-STARRS
por: Tian, Da-Chuan, et al.
Publicado: (2026)

Euclid: Photometric redshift calibration with self-organising maps
por: Roster, W., et al.
Publicado: (2025)

VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability
por: Satheesh-Sheeba, S., et al.
Publicado: (2025)

Improving Photometric Galaxy Clustering Constraints With Cross-Bin Correlations
por: Krywonos, Jordan, et al.
Publicado: (2024)

The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
por: Motta, Pablo, et al.
Publicado: (2026)

Machine Learning Techniques for Astrophysics and Cosmology: Photometric Redshifts
por: Tortorelli, Luca, et al.
Publicado: (2026)

HALO I: Photometric continuum reverberation mapping of Fairall 9
por: Mandal, Amit Kumar, et al.
Publicado: (2025)

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometric Catalog
por: Robertson, Brant E., et al.
Publicado: (2026)

Photometrically Selected Protocluster Candidates at z~9-10 in the JWST COSMOS-Web field
por: Wu, Cossas K. -W., et al.
Publicado: (2025)

The Splashback Mass Function of Galaxy Clusters from Photometric Data
por: Gabriel-Silva, Lucas, et al.
Publicado: (2026)

Inhomogeneous Dust Biases Photometric Redshifts and Stellar Masses for LSST
por: Hahn, ChangHoon, et al.
Publicado: (2024)

TOPz: Photometric redshifts using template fitting applied to the GAMA survey
por: Tempel, E., et al.
Publicado: (2025)

Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
por: Nadler, Ethan O., et al.
Publicado: (2024)

Pz Cats: Photometric redshift catalogs based on DES Y3 BAO sample
por: Ferreira, Paula S., et al.
Publicado: (2025)

A Portrait of the Cosmic Reionisation History in the Context of the Early Dark Energy Model
por: Liu, Weiyang, et al.
Publicado: (2026)

New Insights into Dark Energy from DESI DR2 with CMB and SNIa
por: Qiang, Da-Chun, et al.
Publicado: (2025)

Introducing the DREAMS Project: DaRk mattEr and Astrophysics with Machine learning and Simulations
por: Rose, Jonah C., et al.
Publicado: (2024)

Enhancing Photometric Redshift Catalogs Through Color-Space Analysis: Application to KiDS-Bright Galaxies
por: Jalan, Priyanka, et al.
Publicado: (2024)

Improved constraints on ultralight axions using latest observations of the early and late Universe
por: Liu, Qianshuo, et al.
Publicado: (2025)

Inference of $B$-mode polarization in the presence of non-Gaussian foregrounds
por: Li, Sen, et al.
Publicado: (2025)

NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
por: Ma, Wenlin, et al.
Publicado: (2024)

GLIMPSE-D: An Exotic Balmer-Jump Object at z=6.20? Revisiting Photometric Selection and the Cosmic Abundance of Pop III Galaxies
por: Fujimoto, Seiji, et al.
Publicado: (2025)

Constraints on interacting dark energy revisited: implications for the Hubble tension
por: Hoerning, Gabriel A., et al.
Publicado: (2023)

The COSMOS-Web Lens Survey (COWLS) III: forecasts versus data
por: Hogg, Natalie B., et al.
Publicado: (2025)

Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
por: Chakraborty, Anirban, et al.
Publicado: (2025)

The Dark Energy Camera All Data Everywhere cosmic shear project V: Constraints on cosmology and astrophysics from 270 million galaxies across 13,000 deg$^2$ of the sky
por: Anbajagane, D., et al.
Publicado: (2025)

The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
por: Wang, Yunchong, et al.
Publicado: (2024)

Dark matter distribution in Milky Way-analog galaxies
por: de Isídio, Natanael G., et al.
Publicado: (2023)

Impact of Primordial Black Hole Dark Matter on Gas Properties at Very High Redshift: A Semi-Analytical Model
por: Casanueva-Villarreal, C., et al.
Publicado: (2024)

Early Galaxies and Early Dark Energy: A Unified Solution to the Hubble Tension and Puzzles of Massive Bright Galaxies revealed by JWST
por: Shen, Xuejian, et al.
Publicado: (2024)