Sensitized Molecular Triplet and Triplet Excimer Emission in Two-Dimensional Hybrid Perovskites

2020 ◽  
Vol 11 (6) ◽  
pp. 2247-2255 ◽  
Author(s):  
Yuyang Tian ◽  
Yulu Li ◽  
Baoquan Chen ◽  
Runchen Lai ◽  
Shan He ◽  
...  
1971 ◽  
Vol 11 (4) ◽  
pp. 528-531 ◽  
Author(s):  
O.L.J. Gijzeman ◽  
W.H. van Leeuwen ◽  
J. Langelaar ◽  
J.D.W. van Voorst

1970 ◽  
Vol 5 (5) ◽  
pp. 269-272 ◽  
Author(s):  
O.L.J. Gijzeman ◽  
J. Langelaar ◽  
J.D.W. Van Voorst

1971 ◽  
Vol 11 (4) ◽  
pp. 526-527 ◽  
Author(s):  
O.L.J. Guzeman ◽  
J. Langelaar ◽  
J.D.W. van Voorst

2006 ◽  
Vol 431 (4-6) ◽  
pp. 300-302 ◽  
Author(s):  
M.A. Strzhemechny ◽  
A.A. Avdeenko ◽  
V.V. Eremenko ◽  
O.S. Pyshkin ◽  
L.M. Buravtseva

2011 ◽  
Vol 115 (3) ◽  
pp. 414-421 ◽  
Author(s):  
S. T. Hoffmann ◽  
P. Schrögel ◽  
M. Rothmann ◽  
R. Q. Albuquerque ◽  
P. Strohriegl ◽  
...  

2017 ◽  
Vol 5 (21) ◽  
pp. 5199-5206 ◽  
Author(s):  
Dugang Chen ◽  
Cheng Zhong ◽  
Yan Zhao ◽  
Lingyan Nan ◽  
Yunqi Liu ◽  
...  

A 2D molecule OSPB demonstrated excimer emission in aqueous media and showed high 2PA performance in THF.


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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