“Publications”的版本间差异
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*RR Lyrae in XSTPS: The halo density profile in the North Galactic Cap[http://adsabs.harvard.edu/abs/2014ApJ...788..105F] |
*RR Lyrae in XSTPS: The halo density profile in the North Galactic Cap[http://adsabs.harvard.edu/abs/2014ApJ...788..105F] |
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:L. Faccioli, '''M. C. Smith''' |
:L. Faccioli, '''M. C. Smith''' et al.,2014,ApJ,788,105 |
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*Measuring the X-ray luminosities of SDSS DR7 clusters from ROSAT All Sky Survey[http://adsabs.harvard.edu/abs/2014MNRAS.439..611W] |
*Measuring the X-ray luminosities of SDSS DR7 clusters from ROSAT All Sky Survey[http://adsabs.harvard.edu/abs/2014MNRAS.439..611W] |
2015年2月14日 (六) 05:59的版本
First author
- The Nearest High-velocity Stars Revealed by LAMOST Data Release 1[1]
- Zhong, Jing; Chen, Li et al., ApJ, 2014, 789,2
- The Statistical Nature of the Brightest Group Galaxies [2]
- Shen, Shiyin; Yang, Xiaohu et al., 2014,ApJ,782,23
- Parallaxes of Five L Dwarfs with a Robotic Telescope[3]
- Wang, Y.; Jones, H. R. A.; Smart, R. L.; Marocco, F.; Pinfield, D. J.; Shao, Z. et al., 2014PASP..126...15W
- Properties of abundance gradient along the Galactic disk and the role of LAMOST[4]
- J.L. Hou, L. Chen, J.C. Yu, J. Sellwood and C. Pryor, 2014, IAUS, 298,304
- 星系中球状星团的形成与演化[5]
- 甘建铃,刘成则,沈世银,侯金良, 2014,《天文学进展》, 32, 54
- 阻尼莱曼α吸收线系统研究进展(II)[6]
- 侯金良,尹君,傅承启, 2014, 《天文学进展》,32,182
Coauthors
- An observational and theoretical view of the radial distribution of H I gas in galaxies[7]
- Wang, Jing; Fu, Jian et al., 2014,MNRAS,441,2159
- RR Lyrae in XSTPS: The halo density profile in the North Galactic Cap[8]
- L. Faccioli, M. C. Smith et al.,2014,ApJ,788,105
- Measuring the X-ray luminosities of SDSS DR7 clusters from ROSAT All Sky Survey[9]
- Wang, Lei; Yang, Xiaohu; Shen, Shiyin et al., 2014,MNRAS, 439, 611
- Estimation of absolute magnitude-dependent Galactic model parameters in intermediate latitude with SDSS and SCUSS[10]
- Jia et al., 2014, 441, 503
- A search for double-peaked narrow emission line galaxies and AGNs in the LAMOST DR1[11]
- Shi et al., 2014, RAA, 14, 1234
- Precession of the Sagittarius stream[12]
- Belokurov et al,2014,MNRAS,437,116
- The K Giant Stars from the LAMOST Survey Data. I. Identification, Metallicity, and Distance[13]
- Liu C., et al.,2014,ApJL,790,110