scholarly journals A new approach in separating free from complexed forms of α1-microglobulin and ulinas tatin in human serum

1998 ◽  
Vol 76 ◽  
pp. 133
Author(s):  
Tadahiro Shikimi ◽  
Koichi Kaku ◽  
Hiroshi Ishino ◽  
Hideki Okunishi ◽  
Shuji Takaori
Keyword(s):  
2014 ◽  
Vol 972 ◽  
pp. 14-21 ◽  
Author(s):  
Sussan Ghassabian ◽  
Nur Syazwani Ahmad Rethwan ◽  
Lyn Griffiths ◽  
Maree T. Smith
Keyword(s):  

2008 ◽  
Vol 51 (7) ◽  
pp. 2009-2017 ◽  
Author(s):  
Elisabet Lázaro ◽  
Philip J. Lowe ◽  
Xavier Briand ◽  
Bernard Faller

2015 ◽  
Vol 51 (3) ◽  
pp. 367-373 ◽  
Author(s):  
E. A. Bormotova ◽  
B. L. Mil’man ◽  
T. V. Gupalova

2020 ◽  
Vol 11 (4) ◽  
pp. 1107-1113 ◽  
Author(s):  
Hai-Hao Han ◽  
Adam C. Sedgwick ◽  
Ying Shang ◽  
Na Li ◽  
Tingting Liu ◽  
...  

Herein, we report a protein-based hybridization strategy that exploits the host–guest chemistry of HSA (human serum albumin) to solubilize the otherwise cell impermeable ONOO− fluorescent probe Pinkment-OAc.


2011 ◽  
Vol 100 (3) ◽  
pp. 1142-1146 ◽  
Author(s):  
Michał Piotr Marszałł ◽  
Adam Buciński ◽  
Stefan Kruszewski ◽  
Blanka Ziomkowska

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


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