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   Aghaei, Omid ; Nedimović, Mladen R. ; Marjanović, Milena ; Carbotte, Suzanne M. ; Pablo Canales, J. ; Carton, Hélène ; Nikić, Nikola ( June 2017 , Journal of Geophysical Research: Solid Earth)
2. Transient aspects of the Hadley circulation forced by an idealized off-equatorial ITCZ: TRANSIENT HADLEY CIRCULATION

   https://doi.org/10.1002/2016MS000837  

   Gonzalez, Alex O. ; Mora Rojas, Gabriela ; Schubert, Wayne H. ; Taft, Richard K. ( March 2017 , Journal of Advances in Modeling Earth Systems)
3. Corrected Off-axis Diffraction Holograms for Electrons

   https://doi.org/10.1017/S1431927620014634  

   Pierce, Jordan ; Johnson, Cameron ; McMorran, Benjamin ( August 2020 , Microscopy and Microanalysis)

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4. Enhancing final image contrast in off-axis digital holography using residual fringes

   https://doi.org/10.1364/OE.394231  

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5. Off-axis jet scenario for early afterglow emission of low-luminosity gamma-ray burst GRB 190829A

   https://doi.org/10.1093/mnras/stab1273  

   Sato, Yuri ; Obayashi, Kaori ; Yamazaki, Ryo ; Murase, Kohta ; Ohira, Yutaka ( May 2021 , Monthly Notices of the Royal Astronomical Society)

   null (Ed.)

   ABSTRACT Recently, ground-based Imaging Atmospheric Cherenkov Telescopes have reported the detection of very-high-energy (VHE) gamma-rays from some gamma-ray bursts (GRBs). One of them, GRB 190829A, was triggered by the Swift satellite, and about 2 × 104 s after the burst onset the VHE gamma-ray emission was detected by H.E.S.S. with ∼5σ significance. This event had unusual features of having much smaller isotropic equivalent gamma-ray energy than typical long GRBs and achromatic peaks in X-ray and optical afterglow at about 1.4 × 103 s. Here, we propose an off-axis jet scenario that explains these observational results. In this model, the relativistic beaming effect is responsible for the apparently small isotropic gamma-ray energy and spectral peak energy. Using a jetted afterglow model, we find that the narrow jet, which has the initial Lorentz factor of 350 and the initial jet opening half-angle of 0.015 rad, viewed off-axis can describe the observed achromatic behaviour in the X-ray and optical afterglow. Another wide, baryon-loaded jet is necessary for the later-epoch X-ray and radio emissions. According to our model, the VHE gamma rays observed by H.E.S.S. at 2 × 104 s may come from the narrow jet through the synchrotron self-Compton process. 

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