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researcher

Bin Ma

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.IM1
  • astro-ph.SR1
same name
  • Bin Ma — 8 papers
  • Bin Ma — 6 papers
  • Bin Ma — 5 papers
  • Bin Ma — 4 papers
  • Bin Ma — 3 papers
  • Bin Ma — 2 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.SR2026

A Highly Magnetic Ultra Massive White Dwarf with a 23-minute Rotation Period

Jincheng Guo, Xiaofeng Wang, Qichun Liu +17

We present a physical characterization of TMTS J00063798+3104160 (J0006), a rapidly rotating,ultra-massive white dwarf (WD) identified in high-cadence light curves from the Tsinghu…

astro-ph.GA2025

Discovery of a Luminosity-dependent Continuum Lag in NGC 4151 from Photometric and Spectroscopic Continuum Reverberation Mapping

Hai-Cheng Feng, Sha-Sha Li, Mouyuan Sun +17

Accretion onto supermassive black holes (SMBHs) powers active galactic nuclei (AGNs) and drives feedback that shapes galaxy evolution. Constraining AGN accretion disk structure is…

astro-ph.IM2025

Cosmic Ray Detection and Rejection for CSST

Yan Yu, Bin Ma, Tianmeng Zhang +2

As a space telescope, the China Space Station Survey Telescope (CSST) will face significant challenges from cosmic ray (CR) contamination. These CRs will severely degrade image qua…

astro-ph.GA2025

Optimizing Long-term Variability of AGN Light Curves. I. A Case Study with ZTF Observations in the EGS Field

Jiaqi Lin, Zhen-Ya Zheng, Bin Ma +5

Optical variability is a key observational probe for studying the accretion dynamics and central engine physics of Active Galactic Nuclei (AGNs). The quality and completeness of li…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.