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pro vyhledávání: '"Li, Huabai"'
We present a method for fitting monotone curves using cubic B-splines, which is equivalent to putting a monotonicity constraint on the coefficients. We explore different ways of enforcing this constraint and analyze their theoretical and empirical pr
Externí odkaz:
http://arxiv.org/abs/2307.01748
Autor:
Bryant, Julia J., Motohara, Kentaro, Vernet, Joël R. D., Li, Shaoliang, Bintley, Daniel, Ho, Paul T. P., Lou, Zheng, Chou, Richard C. Y., Furuya, Ray S., Ohashi, Nagayoshi, Doyle, Simon, Li, Huabai, Huang, Junkun, Karoly, Janik, Liu, Kuan-Yu, Singwong, Dan, Oshima, Tai, Kuno, Nario, Honda, Shunsuke, Nakanishi, Hiroyuki, Graves, Sarah, Cookson, Jamie, Chen, Mingtang, Duan, Ran, Ward-Thompson, Derek, Eales, Steve, Barry, Peter, Yu, Shiling, Zhang, Mingzhu, Lv, Weitao, Rujopakarn, Wiphu, Lin, Zhenhui, Shi, Shengcai
Publikováno v:
Proceedings of SPIE; July 2024, Vol. 13096 Issue: 1 p130967K-130967K-17, 12965751p
Publikováno v:
Liu, H. B., Ho, P. T.-P., Zhang, Q., Keto, E., Wu, J. and Li, H. 2010, ApJ, 722, 262-272
This is the first paper of our series of high resolution (1") studies of the massive star forming region G10.6--0.4. We present the emission line observations of the hot core type tracers (O$^{13}$CS, OCS, SO$_{2}$) with $\sim$0$"$.5 resolution. By c
Externí odkaz:
http://arxiv.org/abs/1010.2255
We present a method for fitting monotone curves using cubic B-splines with a monotonicity constraint on the coefficients. We explore different ways of enforcing this constraint and analyze their theoretical and empirical properties. We propose two al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::15f258d87dd30386280fb6f41bc44332
Autor:
Sadaghiani, M., Sánchez-Monge, Álvaro, Schilke, Peter, Liu, Hauyu Baobab, Clarke, S. D., Zhang, Qizhou, Girart, Josep Miquel, Seifried, D., Aghababaei, A., Li, Huabai, Juárez, Carmen, Tang, K. S.
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
[Aims] We aim to characterise certain physical properties of high-mass star-forming sites in the NGC 6334 molecular cloud, such as the core mass function (CMF), spatial distribution of cores, and mass segregation.
[Methods] We used the Atacama L
[Methods] We used the Atacama L
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::61d529f775aa7ab65eb89ffd7a54f938
http://hdl.handle.net/10261/233241
http://hdl.handle.net/10261/233241
Publikováno v:
The Astrophysical Journal; October 2010, Vol. 722 Issue: 1 p262-272, 11p