Conformer analysis and intramolecular excimer formation with the meso and racemic diastereoisomers of 2,4-di(2-pyrenyl)pentane: comparison of NMR and single-photon-counting data

1987 ◽  
Vol 91 (15) ◽  
pp. 3982-3992 ◽  
Author(s):  
Peter. Reynders ◽  
Herbert. Dreeskamp ◽  
Wolfgang. Kuehnle ◽  
Klaas A. Zachariasse
1983 ◽  
Vol 36 (6) ◽  
pp. 1079 ◽  
Author(s):  
E Blatt ◽  
WH Sawyer ◽  
KP Ghiggino

The rotational motions of a set of n-(9-anthroyloxy) fatty acids (n = 2, 6, 9, 12) in dimyristoyl-phosphatidylcholine vesicles above and below the phase transition are investigated. Above the phase transition, single site occupancy and isotropic rotation of the fluorophores allows extraction and comparison of microviscosities from steady-state and time-resolved polarization measurements. Below the phase transition double exponential fluorescence and anisotropy decays are analysed in terms of microheterogeneity of sites. Comparison with previous reports indicates the caution needed when interpreting single photon counting data in terms of hindered rotational motions and order parameters.


1998 ◽  
Vol 145 (4) ◽  
pp. 237 ◽  
Author(s):  
M. Umasuthan ◽  
A.M. Wallace ◽  
J.S. Massa ◽  
G.S. Buller ◽  
A.C. Walker

Author(s):  
Mike Bruce ◽  
Rama R. Goruganthu ◽  
Shawn McBride ◽  
David Bethke ◽  
J.M. Chin

Abstract For time resolved hot carrier emission from the backside, an alternate approach is demonstrated termed single point PICA. The single point approach records time resolved emission from an individual transistor using time-correlated-single-photon counting and an avalanche photo-diode. The avalanche photo-diode has a much higher quantum efficiency than micro-channel plate photo-multiplier tube based imaging cameras typically used in earlier approaches. The basic system is described and demonstrated from the backside on a ring oscillator circuit.


Author(s):  
Maria Concetta Maccarone ◽  
Giovanni La Rosa ◽  
Osvaldo Catalano ◽  
Salvo Giarrusso ◽  
Alberto Segreto ◽  
...  

AbstractUVscope is an instrument, based on a multi-pixel photon detector, developed to support experimental activities for high-energy astrophysics and cosmic ray research. The instrument, working in single photon counting mode, is designed to directly measure light flux in the wavelengths range 300-650 nm. The instrument can be used in a wide field of applications where the knowledge of the nocturnal environmental luminosity is required. Currently, one UVscope instrument is allocated onto the external structure of the ASTRI-Horn Cherenkov telescope devoted to the gamma-ray astronomy at very high energies. Being co-aligned with the ASTRI-Horn camera axis, UVscope can measure the diffuse emission of the night sky background simultaneously with the ASTRI-Horn camera, without any interference with the main telescope data taking procedures. UVscope is properly calibrated and it is used as an independent reference instrument for test and diagnostic of the novel ASTRI-Horn telescope.


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