activity
20232026
most citedUltrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems

9 citations · 9 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

The orbital parameters of gamma-ray binary PSR~J2032+4127

Yu-Feng Luo, Shan-Shan Weng, Qing-Zhong Liu +6

PSR~J2032+4127 is the only one of gamma-ray binary, that exhibits pulsations in gamma-ray. Previous research has indicated that the pulsar and the Be star MT91 213 orbit each other…

astro-ph.GA2026

Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE

Vincenzo R. D'Onofrio, Justin S. Spilker, Rachel Bezanson +10

Many post-starburst galaxies at have been shown to retain substantial molecular gas reservoirs yet host low ongoing star formation, suggesting that the remaining gas may…

astro-ph.GA2025

Searching for Nearby Diffuse Dwarf Galaxies in the COSMOS Field

Dongdong Shi, XianZhong Zheng, Zhizheng Pan +5

It remains challenging to systematically survey nearby diffuse dwarf galaxies and address the formation mechanism of this population distinguishing from regular ones. We carry out…

astro-ph.HE2024★ 9 cited

Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems

The LHAASO Collaboration, Zhen Cao, Felix Aharonian +315

Black holes (BH), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass B…

astro-ph.GA2024

Catalogue of nearby blue and near-solar gas metallicity SDSS dwarf galaxies

Yan Guo, Chandreyee Sengupta, Tom. C. Scott +2

A less explored aspect of dwarf galaxies is their metallicity evolution. Generally, dwarfs have lower metallicities than Hubble sequence late type galaxies but in reality, dwarfs s…

astro-ph.GA2023

HI in high gas-phase metallicity dwarf galaxy WISEA J230615.06+143927.9

Yan Guo, C. Sengupta, T. C. Scott +2

We present resolved GMRT HI observations of the high gas-phase metallicity dwarf galaxy WISEA J230615.06+143927.9 (z = 0.005) (hereafter J2306) and investigate whether it could be…