scholarly journals Controlled and Stable Patterning of Diverse Inorganic Nanocrystals on Crystalline Two-Dimensional Protein Arrays

Biochemistry ◽  
2021 ◽  
Author(s):  
Victor R. Mann ◽  
Francesca Manea ◽  
Nicholas J. Borys ◽  
Caroline M. Ajo-Franklin ◽  
Bruce E. Cohen
2001 ◽  
pp. 330-333 ◽  
Author(s):  
F. G. Tseng ◽  
S. C. Lin ◽  
H. M. Huang ◽  
C. Y. Huang ◽  
C. C. Chieng

Langmuir ◽  
2001 ◽  
Vol 17 (19) ◽  
pp. 5731-5735 ◽  
Author(s):  
Sammy J. Farah ◽  
Szu-Wen Wang ◽  
Wei-Hau Chang ◽  
Channing R. Robertson ◽  
Alice P. Gast

Nano Letters ◽  
2015 ◽  
Vol 15 (8) ◽  
pp. 5235-5239 ◽  
Author(s):  
James F. Matthaei ◽  
Frank DiMaio ◽  
Jeffrey J. Richards ◽  
Lilo D. Pozzo ◽  
David Baker ◽  
...  

2021 ◽  
Vol 10 (2) ◽  
pp. 307-311
Author(s):  
Xiumei Li ◽  
Ruizhen Tian ◽  
Yuancheng Ji ◽  
Shengda Liu ◽  
Xiaojia Jiang ◽  
...  

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.


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