Zobrazeno 1 - 10
of 14 096
pro vyhledávání: '"Jing, Y"'
Publikováno v:
The Astrophysical Journal, Volume 973, 2024, Number 2
Magnification serves as an independent and complementary gravitational lensing measurement to shear. We develop a novel method to achieve an accurate and robust magnification measurement around BOSS CMASS galaxies across physical scales of $0.016h^{-
Externí odkaz:
http://arxiv.org/abs/2405.16484
Autor:
Zheng, Yun, Xu, Kun, Jing, Y. P., Zhao, Donghai, Gao, Hongyu, Luo, Xiaolin, Han, Jiaxin, Yu, Yu, Li, Ming
The roles that mass and environment play in the galaxy quenching are still under debate. Leveraging the Photometric objects Around Cosmic webs (PAC) method, we analyze the excess surface distribution $\bar{n}_2w_{\rm{p}}(r_{\rm{p}})$ of photometric g
Externí odkaz:
http://arxiv.org/abs/2401.11997
Publikováno v:
The Astrophysical Journal, 967:17 (13pp), 2024 May 20
The Photometric objects Around Cosmic webs (PAC) approach developed in Xu et al. (2022b) has the advantage of making full use of spectroscopic and deeper photometric surveys. With the merits of PAC, the excess surface density $\bar{n}_2w_{{\rm{p}}}$
Externí odkaz:
http://arxiv.org/abs/2401.00565
Autor:
Zhang, Chuan-Peng, Zhu, M., Jiang, P., Cheng, C., Wang, J., Xu, J. -L., Liu, X. -L., Yu, N. -P., Qian, L., Yu, H., Ai, M., Jing, Y., Xu, C., Liu, Z., Guan, X., Sun, C., Yang, Q., Huang, M., Hao, Q., Collaboration, FAST
Publikováno v:
Sci. China-Phys. Mech. Astron. 67, 219511 (2024)
The FAST All Sky HI survey (FASHI) was designed to cover the entire sky observable by the Five-hundred-meter Aperture Spherical radio Telescope (FAST), spanning approximately 22000 square degrees of declination between -14 deg and +66 deg, and in the
Externí odkaz:
http://arxiv.org/abs/2312.06097
Autor:
Gao, Hongyu, Jing, Y. P., Xu, Kun, Zhao, Donghai, Gui, Shanquan, Zheng, Yun, Luo, Xiaolin, Aguilar, Jessica Nicole, Ahlen, Steven, Brooks, David, Claybaugh, Todd, Cole, Shaun, de la Macorra, Axel, Forero-Romero, Jaime E., Gontcho, Satya Gontcho A, Ishak, Mustapha, Lambert, Andrew, Landriau, Martin, Manera, Marc, Meisner, Aaron, Miquel, Ramon, Nie, Jundan, Rezaie, Mehdi, Rossi, Graziano, Sanchez, Eusebio, Schubnell, Michael, Seo, Hee-Jong, Tarlé, Gregory, Weaver, Benjamin Alan, Zhou, Zhimin
Galactic conformity is the phenomenon in which a galaxy of a certain physical property is correlated with its neighbors of the same property, implying a possible causal relationship. The observed auto correlations of emission line galaxies (ELGs) fro
Externí odkaz:
http://arxiv.org/abs/2309.03802
Publikováno v:
The Application of Clinical Genetics, Vol Volume 17, Pp 159-169 (2024)
Shuang Lv,1 Yiming Li,2 Bojian Sun,1 Yu Jing,1 Xing Wang,3 Zhanqing Gu,1 Bailiang Wang,4 Cheng Xiao3 1Department of Rheumatology, the First Hospital of Hebei Medical University, Shijiazhuang, Hebei, People’s Republic of China; 2Department of Cardio
Externí odkaz:
https://doaj.org/article/158a3affd89843769afbe22638cdde08
Publikováno v:
International Journal of General Medicine, Vol Volume 17, Pp 4507-4517 (2024)
Yawan Jing,1,2 Ruixin Cheng,3 Hao Zeng,1 Qin Huang,1 Dongyu He,1 Jiayi Sun,1 Panwen Tian,1,4 Yalun Li1,4 1Department of Pulmonary and Critical Care Medicine, State Key Laboratory of Respiratory Health and Multimorbidity, Institute of Respiratory Heal
Externí odkaz:
https://doaj.org/article/61874a4feed143d3bb42c30cd01c1643
Publikováno v:
The Astrophysical Journal, Volume 957, 2023, Number 1
We investigate the alignment of galaxy and halo orientations using the TNG300-1 hydrodynamical simulation. Our analysis reveals that the distribution of the 2D misalignment angle $\theta_{\rm{2D}}$ can be well described by a truncated shifted exponen
Externí odkaz:
http://arxiv.org/abs/2307.12334
The Baryon Acoustic Oscillations (BAO) feature in the clustering of galaxies or quasars provides a ``standard ruler" for distance measurements in cosmology. In this work, we report a $2\sim3\sigma$ signal of the BAO dip feature in the galaxy density-
Externí odkaz:
http://arxiv.org/abs/2306.09407
Autor:
Gao, Hongyu, Jing, Y. P., Gui, Shanquan, Xu, Kun, Zheng, Yun, Zhao, Donghai, Aguilar, Jessica Nicole, Ahlen, Steven, Brooks, David, Claybaugh, Todd, Dawson, Kyle, de la Macorra, Axel, Doel, Peter, Fanning, Kevin, Forero-Romero, Jaime E., Gontcho, Satya Gontcho A, Guy, Julien, Honscheid, Klaus, Kehoe, Robert, Landriau, Martin, Manera, Marc, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Newman, Jeffrey A., Nie, Jundan, Percival, Will, Rossi, Graziano, Schubnell, Michael, Seo, Hee-Jong, Tarlé, Gregory, Weaver, Benjamin Alan, Yu, Jiaxi, Zhou, Zhimin
In the current Dark Energy Spectroscopic Instrument (DESI) survey, emission line galaxies (ELGs) and luminous red galaxies (LRGs) are essential for mapping the dark matter distribution at $z \sim 1$. We measure the auto and cross correlation function
Externí odkaz:
http://arxiv.org/abs/2306.06317