scholarly journals Probing a 2-Aminobenzimidazole Library for Binding to RNA Internal Loops via Two-Dimensional Combinatorial Screening

2012 ◽  
Vol 7 (11) ◽  
pp. 1902-1909 ◽  
Author(s):  
Sai Pradeep Velagapudi ◽  
Alexei Pushechnikov ◽  
Lucas P. Labuda ◽  
Jonathan M. French ◽  
Matthew D. Disney
2011 ◽  
Vol 133 (26) ◽  
pp. 10111-10118 ◽  
Author(s):  
Sai Pradeep Velagapudi ◽  
Steven J. Seedhouse ◽  
Jonathan French ◽  
Matthew D. Disney

Biochemistry ◽  
2008 ◽  
Vol 47 (48) ◽  
pp. 12670-12679 ◽  
Author(s):  
Olga Aminova ◽  
Dustin J. Paul ◽  
Jessica L. Childs-Disney ◽  
Matthew D. Disney

2008 ◽  
Vol 130 (33) ◽  
pp. 11185-11194 ◽  
Author(s):  
Matthew D. Disney ◽  
Lucas P. Labuda ◽  
Dustin J. Paul ◽  
Shane G. Poplawski ◽  
Alexei Pushechnikov ◽  
...  

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.


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