Low-noise Pr3+-doped fluoride fibre amplifier

1995 ◽  
Vol 31 (10) ◽  
pp. 806-807 ◽  
Author(s):  
M. Yamada ◽  
S. Sudo ◽  
Y. Ohishi ◽  
H. Yoshinaga ◽  
K. Oikawa ◽  
...  
Keyword(s):  
1992 ◽  
Vol 28 (20) ◽  
pp. 1924 ◽  
Author(s):  
J.F. Massicott ◽  
R. Wyatt ◽  
B.J. Ainslie

2002 ◽  
Vol 38 (23) ◽  
pp. 1419 ◽  
Author(s):  
A. Mori ◽  
H. Ono ◽  
K. Shikano ◽  
M. Shimizu

1987 ◽  
Vol 23 (19) ◽  
pp. 1026 ◽  
Author(s):  
R.J. Mears ◽  
L. Reekie ◽  
I.M. Jauncey ◽  
D.N. Payne

Author(s):  
Y. Q. Wei ◽  
A. Harsh ◽  
R. V. Penty ◽  
I. H. White ◽  
S. Shen ◽  
...  
Keyword(s):  

1997 ◽  
Vol 33 (9) ◽  
pp. 809 ◽  
Author(s):  
M. Yamada ◽  
Y. Ohishi ◽  
T. Kanamori ◽  
H. Ono ◽  
S. Sudo ◽  
...  

2006 ◽  
Vol 38 (7) ◽  
pp. 625-631
Author(s):  
Shien-Kuei Liaw ◽  
Cheng-Kai Huang ◽  
Yuan–Lung Hsiao ◽  
Li-Chuan Mau ◽  
Hong-Xi Cao ◽  
...  

1996 ◽  
Vol 32 (9) ◽  
pp. 816 ◽  
Author(s):  
J. Massicott ◽  
C. Lebre ◽  
R. Wyatt ◽  
R. Kashyap ◽  
D. Williams ◽  
...  

1988 ◽  
Vol 132 ◽  
pp. 501-506
Author(s):  
C. Sneden ◽  
C. A. Pilachowski ◽  
K. K. Gilroy ◽  
J. J. Cowan

Current observational results for the abundances of the very heavy elements (Z>30) in Population II halo stars are reviewed. New high resolution, low noise spectra of many of these extremely metal-poor stars reveal general consistency in their overall abundance patterns. Below Galactic metallicities of [Fe/H] Ã −2, all of the very heavy elements were manufactured almost exclusively in r-process synthesis events. However, there is considerable star-to-star scatter in the overall level of very heavy element abundances, indicating the influence of local supernovas on element production in the very early, unmixed Galactic halo. The s-process appears to contribute substantially to stellar abundances only in stars more metal-rich than [Fe/H] Ã −2.


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