A fiber-optic-based multichannel time-correlated single-photon-counting device with subnanosecond time resolution

1999 ◽  
Vol 70 (1) ◽  
pp. 32-37 ◽  
Author(s):  
Emanuel Waddell ◽  
Wieslaw J. Stryjewski ◽  
Steven A. Soper
1987 ◽  
Vol 26 (8) ◽  
pp. 1368 ◽  
Author(s):  
R. Stierlin ◽  
J. Ricka ◽  
B. Zysset ◽  
R. Bättig ◽  
Heinz P. Weber ◽  
...  

Four methods of applying mode-locked lasers to time-resolved fluorescence measurements in the subnanosecond region are compared. When time resolution below 100 ps is not required, the most precise and sensitive method is single-photon counting, and the application of this method to studies of time-resolved fluorescence of tryptophan in simple peptides is described. The dependence of lifetimes on pH and temperature are interpreted in terms of quenching by intramolecular proton and electron transfers.


2012 ◽  
Vol 83 (12) ◽  
pp. 123103 ◽  
Author(s):  
Julia Toussaint ◽  
Roman Grüner ◽  
Marco Schubert ◽  
Torsten May ◽  
Hans-Georg Meyer ◽  
...  

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.


Sign in / Sign up

Export Citation Format

Share Document