scholarly journals Polarization-resolved broadband time-resolved optical spectroscopy for complex materials: application to the case of MoTe2 polytypes

2020 ◽  
Vol 28 (6) ◽  
pp. 8819
Author(s):  
Michele Perlangeli ◽  
Simone Peli ◽  
Davide Soranzio ◽  
Denny Puntel ◽  
Fulvio Parmigiani ◽  
...  
Keyword(s):  
Optical Spectroscopy ◽  
Complex Materials ◽  
Time Resolved

Photophysical properties of N719 and Z907 dyes, benchmark sensitizers for dye-sensitized solar cells, at room and low temperature

2021 ◽  
Vol 23 (10) ◽  
pp. 6182-6189
Author(s):  
Dariusz M. Niedzwiedzki
Keyword(s):  
Solar Cells ◽  
Low Temperature ◽  
Optical Spectroscopy ◽  
Room Temperature ◽  
Photophysical Properties ◽  
Dye Sensitized Solar Cells ◽  
Time Resolved ◽  
Dye Sensitized ◽  
Sensitized Solar Cells

Photophysical properties of N719 and Z907, benchmark Ru-dyes used as sensitizers in dye-sensitized solar cells, were studied by static and time-resolved optical spectroscopy at room temperature and 160 K.

scholarly journals Monitoring radiofrequency ablation of biological tissue using broadband time-resolved diffuse optical spectroscopy

2019 ◽  
Author(s):  
Pranav Lanka ◽  
Francis Kalloor Joseph ◽  
Hindrik Kruit ◽  
Sanathana Konugolu Venkata Sekar ◽  
Andrea Farina ◽  
...  
Keyword(s):  
Radiofrequency Ablation ◽  
Optical Spectroscopy ◽  
Biological Tissue ◽  
Time Resolved ◽  
Diffuse Optical Spectroscopy

Scattering delay time of Mie scatterers determined from steady-state and time-resolved optical spectroscopy

2000 ◽  
Vol 17 (4) ◽  
pp. 745
Author(s):  
Stefan Willmann ◽  
Albert Terenji ◽  
Harald Busse ◽  
Ilya V. Yaroslavsky ◽  
Anna N. Yaroslavsky ◽  
...  
Keyword(s):  
Steady State ◽  
Optical Spectroscopy ◽  
Delay Time ◽  
Time Resolved

scholarly journals Chromatic Amplitudes and Line-of-Sight Velocity Variations for the Pulsating DB White Dwarf GD 358

2002 ◽  
Vol 185 ◽  
pp. 380-381
Author(s):  
R. Kotak
Keyword(s):  
Optical Spectroscopy ◽  
White Dwarf ◽  
Line Of Sight ◽  
Time Resolved ◽  
Preliminary Results ◽  
Velocity Variations

AbstractWe report on preliminary results from time-resolved optical spectroscopy of the He-rich variable white dwarf GD 358.

Time-Resolved Optical Spectroscopy as a Probe of Local Polymer Motions

1987 ◽  
pp. 68-82
Author(s):  
Dean A. Waldow ◽  
Patrick D. Hyde ◽  
M. D. Ediger ◽  
Toshiaki Kitano ◽  
Koichi Ito
Keyword(s):  
Optical Spectroscopy ◽  
Time Resolved

Time-resolved optical spectroscopy of IR GEM in quiescence

1991 ◽  
Vol 101 ◽  
pp. 196 ◽  
Author(s):  
C. Lazaro ◽  
I. G. Martinez-Pais ◽  
M. J. Arevalo ◽  
J. E. Solheim
Keyword(s):  
Optical Spectroscopy ◽  
Time Resolved

scholarly journals Carrier dynamics investigated by time resolved optical spectroscopy

2002 ◽  
Vol 32 (2a) ◽  
pp. 353-355
Author(s):  
Saúl J. Luyo ◽  
Maria S.P. Brasil ◽  
Hugo B. de Carvalho ◽  
Wilson de Carvalho Jr. ◽  
Ayrton A. Bernussi
Keyword(s):  
Optical Spectroscopy ◽  
Carrier Dynamics ◽  
Time Resolved

scholarly journals The binary millisecond pulsar PSR J1023+0038 – II. Optical spectroscopy

2019 ◽  
Vol 488 (1) ◽  
pp. 198-212 ◽  
Author(s):  
T Shahbaz ◽  
M Linares ◽  
P Rodríguez-Gil ◽  
J Casares
Keyword(s):  
Radial Velocity ◽  
Optical Spectroscopy ◽  
State Transition ◽  
High Energy ◽  
Accretion Disc ◽  
Millisecond Pulsar ◽  
Mass Ratio ◽  
Time Resolved ◽  
Type Change ◽  
Model Predictions

ABSTRACT We present time-resolved optical spectroscopy of the ‘redback’ binary millisecond pulsar system PSR J1023+0038 during both its radio pulsar (2009) and accretion disc states (2014 and 2016). We provide observational evidence for the companion star being heated during the disc state. We observe a spectral type change along the orbit, from ∼G5 to ∼F6 at the secondary star’s superior and inferior conjunction, respectively, and find that the corresponding irradiating luminosity can be powered by the high-energy accretion luminosity or the spin-down luminosity of the neutron star. We determine the secondary star’s radial velocity semi-amplitude from the metallic (primarily Fe and Ca) and Hα absorption lines during these different states. The metallic and Hα radial velocity semi-amplitude determined from the 2009 pulsar-state observations allows us to constrain the secondary star’s true radial velocity K2 = 276.3 ± 5.6  km s−1 and the binary mass ratio q = 0.137 ± 0.003. By comparing the observed metallic and Hα absorption-line radial velocity semi-amplitudes with model predictions, we can explain the observed semi-amplitude changes during the pulsar state and during the pulsar/disc-state transition as being due to different amounts of heating and the presence of an accretion disc, respectively.

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