High Signal-to-Noise Ratio and Depth Penetration in Time-Domain Functional Near-Infrared Spectroscopy Combining Large Area Detector and High Throughput Electronics

2020 ◽  
Author(s):  
Alberto Dalla Mora ◽  
Laura Di Sieno ◽  
Anurag Behera ◽  
Sumeet Rohilla ◽  
Edoardo Ferocino ◽  
...  
Keyword(s):  
Time Domain ◽  
Near Infrared ◽  
Signal To Noise Ratio ◽  
High Signal ◽  
Large Area ◽  
Signal To Noise ◽  
Functional Near Infrared Spectroscopy ◽  
Area Detector ◽  
Large Area Detector ◽  
Domain Functional

scholarly journals Near-infrared turn-on fluorescent probe for discriminative detection of Cys and application in in vivo imaging

RSC Advances ◽  
2019 ◽  
Vol 9 (71) ◽  
pp. 41431-41437 ◽  
Author(s):  
Shaolong Qi ◽  
Lubao Zhu ◽  
Xinyu Wang ◽  
Jianshi Du ◽  
Qingbiao Yang ◽  
...  
Keyword(s):  
Fluorescent Probes ◽  
Biological Samples ◽  
In Vivo Imaging ◽  
Near Infrared ◽  
Signal To Noise Ratio ◽  
High Signal ◽  
Biological Detection ◽  
Signal To Noise ◽  
Turn On

Near-infrared (NIR) fluorescent probes are widely employed in biological detection because of their lower damage to biological samples, low background interference, and high signal-to-noise ratio.

scholarly journals Multi-channel medical device for time domain functional near infrared spectroscopy based on wavelength space multiplexing

2013 ◽  
Vol 4 (10) ◽  
pp. 2231 ◽  
Author(s):  
Rebecca Re ◽  
Davide Contini ◽  
Massimo Turola ◽  
Lorenzo Spinelli ◽  
Lucia Zucchelli ◽  
...  
Keyword(s):  
Infrared Spectroscopy ◽  
Medical Device ◽  
Near Infrared Spectroscopy ◽  
Time Domain ◽  
Near Infrared ◽  
Functional Near Infrared Spectroscopy ◽  
Domain Functional

scholarly journals High Signal-To-Noise Ratio - the Spectroscopic Key to Algol Systems

1989 ◽  
Vol 107 ◽  
pp. 245-255
Author(s):  
Jocelyn Tomkin
Keyword(s):  
Main Sequence ◽  
Near Infrared ◽  
Signal To Noise Ratio ◽  
Large Fraction ◽  
High Signal ◽  
Signal To Noise ◽  
Algol System ◽  
Low Mass ◽  
Noise Ratio ◽  
Cno Abundances

AbstractThe usefulness of high signal-to-noise-ratio spectra for both radial-velocity and abundance studies of Algol systems is emphasised. It is shown that division by a hot star is a worthwhile step in pursuit of this objective. A preliminary analysis of high signal-to-noise-ratio, red and near-infrared, Reticon observations of R CMa shows that its primary has solar CNO abundances within the 0.3 dex observational error. The low-mass (0.17 m⊙) secondary of this Algol system must have lost a large fraction of its original mass. Some of this material would have been extensively processed during the secondary’s main-sequence lifetime and would therefore have had a highly non-solar CNO-abundance distribution. The lack of serious contamination of the primary’s abundances is consistent with most, but not all, plausible mass-transfer scenarios.

Sign in / Sign up

Export Citation Format

Share Document