activity
20232026
most citedAcceleration of the Universe without the Hubble tension with Kaniadakis holographic dark energy using the Hubble horizon as the IR cut-off

1 citations · 3 across the 18 of their papers we have counts for

collaborators

19 papers

astro-ph.HE2026

A Helical Trajectory Interpretation of a Multi-wavelength Event in a Blazar S5 0716+714

Zhihao Ouyang, Jingyu Wu, Hubing Xiao +9

Relativistic jets in blazars exhibit strong variability across multiple timescales, but the connection between temporal variability and the evolution of jet structures remains poor…

astro-ph.GA2026

Indirect evidence of the extinction bump within the dusty torus of SDSS J141945.50+524648.0

Ze Li, Gaoyang Chen, Qifan Cui +7

We present a multi-wavelength study of the quasar SDSS J141945.50524648.0 (), a member of the newly identified population of quasar-associated $2175\,\mathring{\mathrm…

astro-ph.GA2026

Enhancing Photometric Redshift Estimation for LSST with a Hybrid LSTM-Mixture Density Network

Zhijian Luo, Yangyang Li, Xinyu Luo +4

Accurate photometric redshift (photo-) estimation and robust uncertainty quantification are essential for the LSST to achieve its precision cosmology goals. Traditional machine…

astro-ph.GA2026

Joint constraints on gravity and stellar orbital anisotropy in massive galaxies

Wei Du, Liping Fu, Gong-Bo Zhao +5

Strong gravitational lensing combined with stellar dynamics provides a complementary route for testing gravity on kiloparsec scales and probing the internal structure of massive ga…

astro-ph.GA2026

Beyond Colors: Probing Redshifts from Galaxy Morphology in Single-band Images with ViT-MDNz

Zhijian Luo, Yangyang Li, Jianzhen Chen +5

To address the challenge of estimating redshifts when only single-band images are available, this study introduces a deep learning model named ViT-MDNz. Leveraging robust statistic…

astro-ph.GA2026

First Submillimeter Lights from Dome A: Tracing the Carbon Cycle in the Feedback of Massive Stars

Yan Gong, Jiaqiang Zhong, Yuan Ren +38

The cycling of carbon between its ionized, atomic, and molecular phases shapes the chemical compositions and physical conditions of the interstellar medium (ISM). However, ground-b…

astro-ph.GA2025

LSTM-MDNz: Estimating Quasar Photometric Redshifts with an LSTM-Augmented Mixture Density Network

Jianzhen Chen, Zhijian Luo, Liping Fu +4

Quasar photometric redshifts are essential for studying cosmology and large-scale structures. However, their complex spectral energy distributions cause significant redshift-color…

astro-ph.GA2025

BALNet: Deep Learning-Based Detection and Measurement of Broad Absorption Lines in Quasar Spectra

Yangyang Li, Zhijian Luo, Shaohua Zhang +5

Broad absorption line (BAL) quasars serve as critical probes for understanding active galactic nucleus (AGN) outflows, black hole accretion, and cosmic evolution. To address the li…

astro-ph.GA2025

Identifying Dust-lane Spheroidal Galaxies in DESI Legacy Imaging Surveys Using Semi-Supervised Methods

Zhijian Luo, Jianzhen Chen, Wenxiang Pei +4

Dust-lane spheroidal galaxies (DLSGs) are unique astrophysical systems that exhibit the morphology of early-type galaxies (ETGs) but are distinguished by prominent dust lanes. Rece…

astro-ph.GA2025

Detecting Galactic Rings in the DESI Legacy Imaging Surveys with Semi-Supervised Deep Learning

Jianzhen Chen, Zhijian Luo, Cheng Cheng +3

The ring structures of disk galaxies are vital for understanding galaxy evolution and dynamics. However, due to the scarcity of ringed galaxies and challenges in their identificati…

astro-ph.GA2025

Galaxy Morphology Classification via Deep Semi-Supervised Learning with Limited Labeled Data

Zhijian Luo, Jianzhen Chen, Zhu Chen +4

Galaxy morphology classification plays a crucial role in understanding the structure and evolution of the universe. With galaxy observation data growing exponentially, machine lear…

astro-ph.GA2025

The Quasar-associated 2175 Å Dust Absorbers in the SDSS DR16 Quasar Catalog

Shaohua Zhang, Yuchong Luo, Shangchun Xie +4

We present, for the first time, a systematic study of quasar-associated 2175 Å dust absorbers using spectroscopic data from the Sloan Digital Sky Survey (SDSS) Data Release 16 (DR1…

astro-ph.CO2025

Improving Photometric Redshift Estimation for CSST Mock Catalog Using SED Templates Calibrated with Perturbation Algorithm

Yicheng Li, Liping Fu, Zhu Chen +11

Photometric redshifts of galaxies obtained by multi-wavelength data are widely used in photometric surveys because of its high efficiency. Although various methods have been develo…

astro-ph.GA2024

Photometric Redshift Estimation for CSST Survey with LSTM Neural Networks

Zhijian Luo, Yicheng Li, Junhao Lu +11

Accurate estimation of photometric redshifts (photo-s) is crucial for cosmological surveys. Various methods have been developed for this purpose, such as template fitting method…

astro-ph.IM2024

Cross-Survey Image Transformation: Enhancing SDSS and DECaLS Images to Near-HSC Quality for Advanced Astronomical Analysis

Zhijian Luo, Shaohua Zhang, Jianzhen Chen +5

This study focuses on transforming galaxy images between astronomical surveys, specifically enhancing images from the Sloan Digital Sky Survey (SDSS) and the Dark Energy Camera Leg…

astro-ph.GA2024★ 1 cited

A comparative study of ultraluminous infrared galaxies in the IRAS and SDSS Surveys

Shaohua Zhang, Zhijian Luo, Xiheng Shi +3

We present a comprehensive study of Ultraluminous Infrared Galaxies (ULIRGs), leveraging data from the IRAS Faint Source Catalogue (FSC) and the spectroscopic catalog in the Sloan…

astro-ph.CO2024★ 1 cited

Acceleration of the Universe without the Hubble tension with Kaniadakis holographic dark energy using the Hubble horizon as the IR cut-off

Wei Fang, Guo Chen, Chao-Jun Feng +2

We introduce a holographic dark energy model that incorporates the first-order approximate Kaniadaski entropy, utilizing the Hubble horizon, , as the infrared cutoff. We inves…

astro-ph.IM2024

Imputation of Missing Photometric Data and Photometric Redshift Estimation for CSST

Zhijian Luo, Zhirui Tang, Zhu Chen +10

Accurate photometric redshift (photo-) estimation requires support from multi-band observational data. However, in the actual process of astronomical observations and data proce…

astro-ph.CO2023★ 1 cited

Estimating Photometric Redshift from Mock Flux for CSST Survey by using Weighted Random Forest

Junhao Lu, Zhijian Luo, Zhu Chen +10

Accurate estimation of photometric redshifts (photo-) is crucial in studies of both galaxy evolution and cosmology using current and future large sky surveys. In this study, we…