activity
19972023
most citedPulse Profiles, Spectra and Polarization Characteristics of Non-Thermal Emissions from the Crab-Like Pulsars

69 citations · 560 across the 50 of their papers we have counts for

collaborators
Showing 2017Show all

5 papers · 1 filter

astro-ph.HE2017★ 7 cited

Searching for High Energy, Horizon-scale Emissions from Galactic Black Hole Transients during Quiescence

Lupin Chun-Che Lin, Hung-Yi Pu, Kouichi Hirotani +5

We search for the gamma-ray counterparts of stellar-mass black holes using long-term Fermi archive to investigate the electrostatic acceleration of electrons and positrons in the v…

astro-ph.GA2017★ 5 cited

Enhanced gamma radiation toward the rotation axis from the immediate vicinity of extremely rotating black holes

Yoogeun Song, Hung-Yi Pu, Kouichi Hirotani +3

We investigate the acceleration of electrons and positrons by magnetic-field-aligned electric fields in the polar funnel of an accreting black hole (BH). Applying the pulsar outer-…

astro-ph.HE2017★ 19 cited

Lepton acceleration in the vicinity of the event horizon: Very-high-energy emissions from super-massive black holes

Kouichi Hirotani, Hung-Yi Pu, Lupin Chun-Che Lin +5

Around a rapidly rotating black hole (BH), when the plasma accretion rate is much less than the Eddington rate, the radiatively inefficient accretion flow (RIAF) cannot supply enou…

astro-ph.IM2017

Benchmarking COSI's detector effects engine

Clio C. Sleator, Steven E. Boggs, Jeng-Lun Chiu +11

The Compton Spectrometer and Imager (COSI) is a balloon-borne gamma-ray (0.2-5 MeV) telescope with inherent sensitivity to polarization. COSI's main goal is to study astrophysical…

astro-ph.IM2017★ 8 cited

The 2016 Super Pressure Balloon flight of the Compton Spectrometer and Imager

Carolyn A. Kierans, Steven E. Boggs, Jeng-Lun Chiu +11

The Compton Spectrometer and Imager (COSI) is a balloon-borne, soft-gamma ray imager, spectrometer, and polarimeter with sensitivity from 0.2 to 5 MeV. Utilizing a compact Compton…