collaborators

6 papers

astro-ph.GA2026

Search for quasar pairs with Gaia astrometric data. II. Photometric redshift prediction with machine learning for the MGQPC catalogue

Xingyu Zhu, Qihang Chen, Liang Jing +4

The identification of physically associated kiloparsec-scale quasar pairs is important for understanding galaxy evolution, the growth of supermassive black holes, and their co-evol…

astro-ph.GA2026

Photometric Redshift PDFs via Neural Network Classification for DESI Legacy Imaging Surveys and Pan-STARRS

Da-Chuan Tian, Zhong-Lue Wen, Jun-Qing Xia

We present a neural network classification (NNC) method for photometric redshift estimation that produces well-calibrated redshift probability density functions (PDFs). The method…

astro-ph.GA2026

A Quasar Pair Sample Compiled from DESI DR1

Liang Jing, Qihang Chen, Zhuojun Deng +4

Interacting quasar pairs (QPs, either dual or binary) provide crucial insights into galaxy mergers, black hole growth, and large-scale structure formation. The current literature r…

astro-ph.CO2025

Do JWST reionization (optical depth) puzzle, cosmological tensions, and CMB anomalies imply Harrison-Zel'dovich spectrum?

Hao-Hao Li, Xin-zhe Zhang, Taotao Qiu +1

The James Webb Space Telescope (JWST) has observed massive galaxies at high redshifts, which implies an earlier epoch of reionization (EoR) compared with the cosmic microwave backg…

astro-ph.CO2025

Measuring Cosmic Growth Rate with CSST Spectroscopic Survey and Fast Radio Burst

Shi-Yuan Wang, Jun-Qing Xia

The cosmic growth rate, which is related to peculiar velocity and is a primary scientific objective of galaxy spectroscopic surveys, can be inferred from the Redshift Space Distort…

astro-ph.CO2025

Constraints on Evolutions of Fundamental Constants from Clustering of Fast Radio Burst Dispersion Measure

Shi-Yuan Wang, Jun-Qing Xia

Constrained measurements of fundamental physical constants using astronomical observational data represent a powerful method for investigating potential new physics. In particular,…