activity
20162023
most citedPhysical properties of CO-dark molecular gas traced by C

29 citations · 122 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2023★ 7 cited

Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534

Chen-Chen Miao, Victoria Blackmon, Wei-Wei Zhu +41

We report the radio observations of the eclipsing black widow pulsar J1720-0534, a 3.26 ms pulsar in orbit with a low mass companion of mass 0.029 to 0.034 M. We obtain t…

astro-ph.HE2023★ 24 cited

An extremely active repeating fast radio burst source in a likely non-magneto-ionic environment

Yi Feng, Di Li, Yong-Kun Zhang +24

Fast radio bursts (FRBs) are bright radio bursts originating at cosmological distances. Only three repeating FRBs FRB 20121102A, FRB 20190520B and FRB 20201124A among 60 kno…

astro-ph.GA2020★ 9 cited

Hyperfine Group Ratio: A Recipe for Deriving Kinetic Temperature from Ammonia Inversion Lines

Shen Wang, Zhiyuan Ren, Di Li +3

Although ammonia is a widely used interstellar thermometer, the estimation of its rotational and kinetic temperatures can be affected by the blended Hyperfine Components (HFCs). We…

astro-ph.GA2020★ 8 cited

Filament Intersections and Cold Dense Cores in Orion A North

Chao Zhang, Zhiyuan Ren, Jingwen Wu +13

We studied the filament structures and dense cores in OMC-2,3 region in Orion A North molecular cloud using the high-resolution N2H+ (1-0) spectral cube observed with the Atacama L…

astro-ph.IM2019★ 16 cited

A PRESTO-based Parallel Pulsar Search Pipeline Used for FAST Drift Scan Data

Qiuyu Yu, Zhichen Pan, Lei Qian +9

We developed a pulsar search pipeline based on PRESTO (PulsaR Exploration and Search Toolkit). This pipeline simply runs dedispersion, FFT (Fast Fourier Transformation), and accele…

astro-ph.HE2019★ 2 cited

Probing the emission states of PSR J1107-5907

Jingbo Wang, George Hobbs, Matthew Kerr +14

The emission from PSR J1107-5907 is erratic. Sometimes the radio pulse is undetectable, at other times the pulsed emission is weak, and for short durations the emission can be very…