activity
19962026
most citedPah and Mid-IR Luminosities as Measures of Star-Formation Rate in Spitzer First Look Survey Galaxies

233 citations · 3.3k across the 99 of their papers we have counts for

collaborators

100 papers

astro-ph.GA2026

Inside-out growth and the kiloparsec-scale star formation main sequence for low-surface-brightness disk galaxies in MaNGA

Bing-qing Zhang, Ze-hao Zhong, Yi-nan Zhu +1

Low surface brightness galaxies (LSBGs) are very faint objects in the universe whose formation and evolution have long remained an unresolved problem. We selected a late-type, face…

astro-ph.GA2023★ 11 cited

Understanding the chemical evolution of blue Edge-on Low Surface Brightness Galaxies

Tian-wen Cao, Hong Wu, Gaspar Galaz +4

We present a sample of 330 blue edge-on low surface brightness galaxies (ELSBGs). To understand the chemical evolution of LSBGs, we derived the gas-phase abundance and the [/Fe]…

astro-ph.GA2022★ 4 cited

Radio continuum and OH line emission of high-z OH megamaser galaxies

Zhongzu Wu, Yu. V. Sotnikova, Bo Zhang +8

We present the study of arcsecond scale radio continuum and OH line emission of a sample of known OH megamaser galaxies with 0.15 using archival Very Large Array (VLA) dat…

astro-ph.HE2022★ 10 cited

Optical Observations of the Nearby Type Ia Supernova 2021hpr

Yu Zhang, Tianmeng Zhang, Danzengluobu +6

We present the optical photometric and spectroscopic observations of the nearby Type Ia supernova (SN) 2021hpr. The observations covered the phase of 14.37 to +63.68 days relati…

astro-ph.IM2022★ 24 cited

Automatic detection of low surface brightness galaxies from SDSS images

Zhenping Yi, Jia Li, Wei Du +7

Low surface brightness (LSB) galaxies are galaxies with central surface brightness fainter than the night sky. Due to the faint nature of LSB galaxies and the comparable sky backgr…

astro-ph.GA2022★ 8 cited

Radio properties of the OH megamaser galaxy IIZw 096

Hong Wu, Zhongzu Wu, Yu. Sotnikova +9

Based on the two epochs EVN archive data from OH line observations of IIZw 096, we confirm that the high-resolution OH emission in this source mainly comes from two spots (OH1 and…