Image de couverture de livre

ASTROFLOW: A Real-Time End-to-End Pipeline for Radio Single-Pulse Searches

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Lin, Guanhong, Zhou, Dejia, Zhang, Jianli, Ding, Jialang, Liu, Fei, Ma, Xiaoyun, Liang, Yuan, Duan, Ruan, Liu, Liaoyuan, Wang, Xuanyu, Yan, Xiaohui, Zhan, Yingrou, Chu, Yuting, Qiao, Jing, Wang, Wei, Zhang, Jie, Wang, Zerui, Liu, Meng, Miao, Chenchen, Liu, Menquan, Guo, Meng, Li, Di, Wang, Pei
Format:	Preprint
Publié:	2025
Sujets:	Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

A Python/CuPy Software Correlator for QUEST: Real-Time Performance and Initial Imaging
par: Ding, Jialang, et autres
Publié: (2026)

The long-term evolution of the GW170817 remnant
par: Liu, Menquan, et autres
Publié: (2024)

Dynamical Mass Loss at the End of TP-AGB stars
par: Cui, Yingzhen, et autres
Publié: (2026)

Discovery of a millisecond pulsar with a CO white dwarf companion
par: Zhang, Jie, et autres
Publié: (2026)

Detection of HI filament: Pair Stacking vs. Filament Stacking
par: Meng, Yuxi, et autres
Publié: (2025)

BLINK: an End-To-End GPU High Time Resolution Imaging Pipeline for Fast Radio Burst Searches with the Murchison Widefield Array
par: Di Pietrantonio, Cristian, et autres
Publié: (2025)

Mock Observations for the CSST Mission: End-to-End Performance Modeling of Optical System
par: Ban, Zhang, et autres
Publié: (2025)

SN2024abfl: A Low-Luminosity Type IIP Supernova at the Low-Mass End of Core Collapse
par: Li, Luhan, et autres
Publié: (2026)

HiFAST: An HI Data Calibration and Imaging Pipeline for FAST III. Standing Wave Removal
par: Xu, Chen, et autres
Publié: (2024)

Towards a foundation model for astrophysical source detection: An End-to-End Gamma-Ray Data Analysis Pipeline Using Deep Learning
par: Pérez-Romero, Judit, et autres
Publié: (2025)

Neuromorphic Astronomy: An End-to-End SNN Pipeline for RFI Detection Hardware
par: Pritchard, Nicholas J., et autres
Publié: (2025)

GRM Scientific Pipeline
par: Wang, Ping, et autres
Publié: (2026)

Forecasting Supernova Observations with the CSST: I. Photometric Samples
par: Liu, Chengqi, et autres
Publié: (2024)

DRAFTS: A Deep Learning-Based Radio Fast Transient Search Pipeline
par: Zhang, Yong-Kun, et autres
Publié: (2024)

Propagation-induced Frequency-dependent Polarization Properties of Fast Radio Burst
par: Wang, Wei-Yang, et autres
Publié: (2025)

A Generalist Model Including Evolved Star Mass and Age
par: Zhang, Mengmeng, et autres
Publié: (2026)

Toward the End-To-End Optimization of the SWGO Array Layout
par: Dorigo, Tommaso, et autres
Publié: (2023)

Back-End System of BURSTT
par: Lin, Kai-Yang, et autres
Publié: (2025)

Fermi detection of gamma-ray Emission from the Hot Coronae of Radio-quiet Active Galactic Nuclei
par: Liu, Jun-Rong, et autres
Publié: (2025)

Observation of HI around three satellite galaxies of the M31 with the FAST: Andromeda II, NGC 205, and NGC 185
par: Liu, Ziming, et autres
Publié: (2024)

Discovery of Main-sequence Radio Pulse emitters from widefield sky surveys
par: Das, Barnali, et autres
Publié: (2025)

CSST Large-scale Structure Analysis Pipeline: II. the CSST Emulator for Slitless Spectroscopy (CESS)
par: Wen, Run, et autres
Publié: (2024)

The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
par: Liu, Zhenjie, et autres
Publié: (2024)

Machine Phenomenology: A Simple Equation Classifying Fast Radio Bursts
par: Liu, Yang, et autres
Publié: (2025)

Supernova Classification using the Recurrent Neural Network in the CSST Ultra-Deep Field Survey
par: Wang, Minglin, et autres
Publié: (2025)

Investigating the Anisotropy of Dispersion Measure Contribution from the Galactic Halo by Using Fast Radio Bursts
par: Liu, Yang, et autres
Publié: (2026)

Bounding the Photon Mass with Ultrawide Bandwidth Pulsar Timing Data and Dedispersed Pulses of Fast Radio Bursts
par: Wang, Yu-Bin, et autres
Publié: (2024)

Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
par: Wang, Xinghuan, et autres
Publié: (2025)

Radio AGN feedback sustains quiescence only in a minority of massive galaxies
par: Liu, Huiling, et autres
Publié: (2025)

Using End-to-End Optimized Summary Statistics to Improve IceCube's Diffuse Galactic Fits
par: Janik, Oliver, et autres
Publié: (2025)

End-to-End Lyapunov-Based Eclipse-Feasible Low-Thrust Transfer Trajectories to NRHO
par: Nurre, Nicholas P., et autres
Publié: (2024)

A Differentiable, End-to-End Forward Model for 21 cm Cosmology: Estimating the Foreground, Instrument, and Signal Joint Posterior
par: Kern, Nicholas
Publié: (2025)

RG-CAT: Detection Pipeline and Catalogue of Radio Galaxies in the EMU Pilot Survey
par: Gupta, Nikhel, et autres
Publié: (2024)

Polarization Profiles of Globular Cluster Pulsars from FAST I. 25 Profiles from Previously Known Pulsars
par: Liu, Tong, et autres
Publié: (2025)

What are recent observations telling us in light of improved tests of distance duality relation?
par: Tonghua, Liu, et autres
Publié: (2023)

Large-scale Array for Radio Astronomy on the Farside
par: Chen, Xuelei, et autres
Publié: (2024)

A Portrait of the Cosmic Reionisation History in the Context of the Early Dark Energy Model
par: Liu, Weiyang, et autres
Publié: (2026)

CosmicWeb-21cm array: A New Radio Observation Array Design for 21cm Cosmology
par: Wang, Jiancheng, et autres
Publié: (2026)

Searching for accreting compact binary systems from spectroscopy and photometry: Application to LAMOST spectra
par: Zhao, Xinlin, et autres
Publié: (2025)

End-to-End simulation framework for astronomical spectrographs: SOXS, CUBES and ANDES
par: Scaudo, A., et autres
Publié: (2024)