Difference between revisions of "Publications"
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*The evolution of interacting spiral galaxy NGC 5194[http://adsabs.harvard.edu/abs/2015MNRAS.449..414K] | *The evolution of interacting spiral galaxy NGC 5194[http://adsabs.harvard.edu/abs/2015MNRAS.449..414K] | ||
:Kang, Xiaoyu; Chang, Ruixiang; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414 | :Kang, Xiaoyu; Chang, Ruixiang; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414 | ||
*Using member galaxy luminosities as halo mass proxies of galaxy groups [http://adsabs.harvard.edu/abs/2015ApJ...804...55L] | |||
:Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2015ApJ...804...55L | |||
*Capability of Quasar Selection by Combining SCUSS and SDSS Observations [http://adsabs.harvard.edu/abs/2015PASP..127...94Z] | *Capability of Quasar Selection by Combining SCUSS and SDSS Observations [http://adsabs.harvard.edu/abs/2015PASP..127...94Z] | ||
:Zhou H. et al., 2015,PASP,127,94 | :Zhou H. et al., 2015,PASP,127,94 | ||
Revision as of 01:12, 11 May 2015
- An Apparent Redshift Dependence of Quasar Continuum: Implication for Cosmic Dust Extinction? [1]
- Xie, Xiaoyi; Shen, Shiyin; Shao, Zhengyi; Yin, Jun, 2015, ApJL, 802,16
- The evolution of interacting spiral galaxy NGC 5194[2]
- Kang, Xiaoyu; Chang, Ruixiang; Zhang, Fenghui; Cheng, Liantao; Wang,Lang,2015,MNRAS,449,414
- Using member galaxy luminosities as halo mass proxies of galaxy groups [3]
- Lu, Yi; Yang, Xiaohu; Shen, Shiyin, 2015ApJ...804...55L
- Capability of Quasar Selection by Combining SCUSS and SDSS Observations [4]
- Zhou H. et al., 2015,PASP,127,94
- An Investigation of the Absolute Proper Motions of the SCUSS Catalog[5]
- Peng, Xiyan et al., 2015, PASP, 127, 250[]