Zobrazeno 1 - 10
of 1 451
pro vyhledávání: '"SHI Jingjing"'
Autor:
CHEN Xuanyi, SHI Jingjing, ZHANG Xiangqian, LU Zhanyuan, GE Guolong, DU Xiangyu, CHEN Lirong, HAO Yonghe
Publikováno v:
Guan'gai paishui xuebao, Vol 43, Iss 9, Pp 39-48 (2024)
【Objective】 Maize is a main staple crop cultivated in central and Northern China but it requires irrigation at certain stages during its growth. In this paper, we present the findings of an experimental study on the effect of irrigation amount on
Externí odkaz:
https://doaj.org/article/a036aed34a5845c7aefb561d7704195e
Autor:
SHI Jingjing, LAN Huiqing, ZHANG Xiangqian, LU Zhanyuan, BU Hengtong, BAI Dongxing, CHENG Yuchen, DU Xiangyu, WANG Manxiu, CHEN Xuanyi
Publikováno v:
Guan'gai paishui xuebao, Vol 42, Iss 9, Pp 1-8 (2023)
【Objective】 The purpose of this paper is to investigate the effect of drip irrigation amount on dry matter accumulation and distribution, as well as the yield formation of the grain machine harvest maize. 【Method】 The study was based on the d
Externí odkaz:
https://doaj.org/article/40e019a614254d13aea6d3ca831c6321
Autor:
Hoque, Md Shafkat Bin, Liao, Michael E., Zare, Saman, Liu, Zeyu, Koh, Yee Rui, Huynh, Kenny, Shi, Jingjing, Graham, Samuel, Luo, Tengfei, Ahmad, Habib, Doolittle, W. Alan, Goorsky, Mark S., Hopkins, Patrick E.
Bulk AlN possesses high thermal conductivity due to long phonon mean-free-paths, high group velocity, and long lifetimes. However, the thermal transport scenario becomes very different in a thin AlN film due to phonon-defect and phonon-boundary scatt
Externí odkaz:
http://arxiv.org/abs/2409.14328
We perform a thorough analysis of the projected shapes of nearby galaxies in both observations and cosmological simulations. We implement a forward-modeling approach to overcome the limitations in previous studies, which hinder accurate comparisons b
Externí odkaz:
http://arxiv.org/abs/2407.19152
Autor:
Sunayama, Tomomi, Miyatake, Hironao, Sugiyama, Sunao, More, Surhud, Li, Xiangchong, Dalal, Roohi, Rau, Markus Michael, Shi, Jingjing, Chiu, I-Non, Shirasaki, Masato, Zhang, Tianqing, Nishizawa, Atsushi J.
We present cosmology results obtained from a blind joint analysis of the abundance, projected clustering, and weak lensing of galaxy clusters measured from the Sloan Digital Sky Survey (SDSS) redMaPPer cluster catalog and the Hyper-Suprime Cam (HSC)
Externí odkaz:
http://arxiv.org/abs/2309.13025
Autor:
Lamman, Claire, Tsaprazi, Eleni, Shi, Jingjing, Šarčević, Nikolina Niko, Pyne, Susan, Legnani, Elisa, Ferreira, Tassia
We summarize common notations and concepts in the field of Intrinsic Alignments (IA). IA refers to physical correlations involving galaxy shapes, galaxy spins, and the underlying cosmic web. Its characterization is an important aspect of modern cosmo
Externí odkaz:
http://arxiv.org/abs/2309.08605
Autor:
Bottrell, Connor, Yesuf, Hassen M., Popping, Gergö, Omori, Kiyoaki Christopher, Tang, Shenli, Ding, Xuheng, Pillepich, Annalisa, Nelson, Dylan, Eisert, Lukas, Gao, Hua, Goulding, Andy D., Kalita, Boris S., Luo, Wentao, Greene, Jenny E., Shi, Jingjing, Silverman, John D.
At fixed galaxy stellar mass, there is a clear observational connection between structural asymmetry and offset from the star forming main sequence, $\Delta$SFMS. Herein, we use the TNG50 simulation to investigate the relative roles of major mergers
Externí odkaz:
http://arxiv.org/abs/2308.14793
Autor:
Shi, Jingjing, Sunayama, Tomomi, Kurita, Toshiki, Takada, Masahiro, Sugiyama, Sunao, Mandelbaum, Rachel, Miyatake, Hironao, More, Surhud, Nishimichi, Takahiro, Johnston, Harry
Galaxy clusters, being the most massive objects in the Universe, exhibit the strongest alignment with the large-scale structure. However, mis-identification of members due to projection effects from the large scale structure can occur. We studied the
Externí odkaz:
http://arxiv.org/abs/2306.09661
Autor:
Zhang, Benjamin, Lee, Khee-Gan, Krolewski, Alex, Shi, Jingjing, Horowitz, Benjamin, Kooistra, Robin
Galaxy formation theories predict that galaxy shapes and angular momenta have non-random alignments with the cosmic web. This leads to so-called intrinsic alignment between pairs of galaxies, which is important to quantify as a nuisance parameter for
Externí odkaz:
http://arxiv.org/abs/2211.09331
Autor:
Shi, Jingjing, Zhang, Siying, Xiao, Mengyao, Wang, Na, Hu, Panpan, Shi, Jiping, Tang, Tao, Liu, Li
Publikováno v:
In Chemical Engineering Journal 15 October 2024 498