CL
C. -J. Li
astro-ph.HEastro-ph.SRastro-ph.GAastro-ph.IMastro-ph.COphysics.ins-det
On Valency
published · living versionsW_tkh7xznc·v1 · currentpublished
Performance of two Askaryan Radio Array stations and first results in the search for ultra-high energy neutrinos
with ARA Collaboration, P. Allison, R. Bard, J. J. Beatty +62
1 version
W_uhcs9wfb·v1published
Preprints & journals
20 papers in the corpus · 2014–2026A MUSE View of the Optical Torus within the Supernova Remnant 1E 0102.2-72192606.17563v1 · Janette Suherli, Samar Safi-Harb, Ivo R. Seitenzahl et al.2026 · 0 citationsarXiv
Intertwined birth and death: a Herbig-Haro outflow resolves the distance to Vela Junior2512.04956v1 · Janette Suherli, Ivo R. Seitenzahl, Samar Safi-Harb et al.2025 · 3 citationsarXiv
The Altered Chaplygin Model as a Model for Dark Energy2509.14826v2 · Yi-Syuan Wu, Chuan-Jui Li, W. F. Kao2025 · 0 citationsarXiv
The Dark Energy Camera Magellanic Clouds Emission-Line Survey2409.04846v1 · Sean D. Points, Knox S. Long, William P. Blair et al.2024 · 7 citationsarXiv
Stellar Population near NGC 2021: Procession of Star Formation in the South Rim of Supergiant Shell LMC 42405.04024v1 · Po-Sheng Ou, Rui-Ching Chao, You-Hua Chu et al.2024 · 2 citationsarXiv
MUSE observations of the optical nebula surrounding the central compact object in the Vela Junior Supernova Remnant2311.17206v1 · Janette Suherli, Samar Safi-Harb, Ivo R. Seitenzahl et al.2023 · 1 citationarXiv
New Insights on 30 Dor B Revealed by High-Quality Multi-wavelength Observations2309.13313v1 · Wei-An Chen, Chuan-Jui Li, You-Hua Chu et al.2023 · 3 citationsarXiv
The Shellless SNR B0532-67.5 in the Large Magellanic Cloud2111.02900v2 · Chuan-Jui Li, You-Hua Chu, Chen-Yu Chuang et al.2021 · 4 citationsarXiv
Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-Dominated Shells2110.09250v2 · Chuan-Jui Li, You-Hua Chu, John C. Raymond et al.2021 · 14 citationsarXiv
SN 2018bsz: significant dust formation in a nearby superluminous supernova2109.07942v2 · T.-W. Chen, S. J. Brennan, R. Wesson et al.2021 · 10 citationsarXiv
Searching for Surviving Companion in the Young SMC Supernova Remnant 1E 0102.2-72192104.04835v2 · Chuan-Jui Li, Ivo R. Seitenzahl, Ryoko Ishioka et al.2021 · 3 citationsarXiv
A Multiwavelength Survey of Wolf-Rayet Nebulae in the Large Magellanic Cloud2101.01622v1 · Clara Shang Hung, Po-Sheng Ou, You-Hua Chu et al.2021 · 11 citationsThe Astrophysical Journal Supplement Series, Volume 252, Issue 2, id.21, 2021
Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations1912.00987v2 · P. Allison, S. Archambault, J.J. Beatty et al.2019 · 74 citationsPhys. Rev. D 102, 043021 (2020)
Recent Results from The Askaryan Radio Array1907.11125v1 · P. Allison, S. Archambault, R. Bard et al.2019 · 2 citationsarXiv
Design and Performance of an Interferometric Trigger Array for Radio Detection of High-Energy Neutrinos1809.04573v2 · P. Allison, S. Archambault, R. Bard et al.2018 · 66 citationsarXiv
Measurement of the real dielectric permittivity epsilon_r of glacial ice1712.03301v2 · P. Allison, S. Archambault, J. Auffenberg et al.2017 · 2 citationsarXiv
Physical Structures of the Type Ia Supernova Remnant N103B1701.05852v1 · Chuan-Jui Li, You-Hua Chu, Robert A. Gruendl et al.2017 · 24 citationsThe Astrophysical Journal, Volume 836, Number 1, 2017
Performance of two Askaryan Radio Array stations and first results in the search for ultra-high energy neutrinos1507.08991v3 · P. Allison, R. Bard, J. J. Beatty et al.2015 · 142 citationsPhys. Rev. D 93, 082003 (2016)on Valency
Constraints on the Ultra-High Energy Neutrino Flux from Gamma-Ray Bursts from a Prototype Station of the Askaryan Radio Array1507.00100v2 · P. Allison, J. Auffenberg, R. Bard et al.2015 · 8 citationsAstropart.Phys. 88 (2017) 7-16
First Constraints on the Ultra-High Energy Neutrino Flux from a Prototype Station of the Askaryan Radio Array1404.5285v3 · P. Allison, J. Auffenberg, R. Bard et al.2014 · 76 citationsarXivon Valency
Career total: 33 works. 20 are in this corpus.
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