Simultaneous Analysis of Hundreds of Y-Chromosomal SNPs for High-Resolution Paternal Lineage Classification using Targeted Semiconductor Sequencing

2014 ◽  
Vol 36 (1) ◽  
pp. 151-159 ◽  
Author(s):  
Arwin Ralf ◽  
Mannis van Oven ◽  
Kaiyin Zhong ◽  
Manfred Kayser
2013 ◽  
Vol 9 (S301) ◽  
pp. 499-500
Author(s):  
Nathalie Themessl ◽  
Veronique Fritz ◽  
Michel Breger ◽  
Sabine Karrer ◽  
Barbara G. Castanheira

AbstractOur simultaneous analysis of ground-based photometric and high-resolution spectroscopic data of the δ Scuti star V376 Per revealed eight individual frequencies from 82 nights of two-color photometry and six frequencies from the line-profile variations using 769 stellar spectra. Additionally, we identified the corresponding pulsation modes and derived reliable estimates of the line profile and pulsation mode parameters.


1982 ◽  
Vol 3 (1) ◽  
pp. 83-95 ◽  
Author(s):  
F. Meyer ◽  
J. Dupré ◽  
C. Meyer ◽  
C. Lambeau ◽  
M. De Vleeschouwer ◽  
...  

The Analyst ◽  
2019 ◽  
Vol 144 (1) ◽  
pp. 220-229 ◽  
Author(s):  
Michaela Schwaiger ◽  
Harald Schoeny ◽  
Yasin El Abiead ◽  
Gerrit Hermann ◽  
Evelyn Rampler ◽  
...  

Dual HILIC and RP chromatography coupled to high-resolution mass spectrometry for the simultaneous analysis of metabolites and lipids.


Author(s):  
R. Ruscica ◽  
R. Wolf ◽  
D. Evins

A logical extension of applications of the Scanning Electron Microscope is the area of x-ray analysis. The instrument utilized is the Materials Analysis Company Model 700 High Resolution Scanning Electron Microscope equipped with a fully focusing dispersive spectrometer and a Solid-State nondispersive spectrometer. The instrument can be equipped with both accessories so that simultaneous analysis with both systems is possible.


2019 ◽  
Vol 83 (1) ◽  
pp. 53-64 ◽  
Author(s):  
Siti U. Mokhtar ◽  
Chadin Kulsing ◽  
Jalal T. Althakafy ◽  
Alex Kotsos ◽  
Olaf H. Drummer ◽  
...  

1967 ◽  
Vol 31 ◽  
pp. 45-46
Author(s):  
Carl Heiles

High-resolution 21-cm line observations in a region aroundlII= 120°,b11= +15°, have revealed four types of structure in the interstellar hydrogen: a smooth background, large sheets of density 2 atoms cm-3, clouds occurring mostly in groups, and ‘Cloudlets’ of a few solar masses and a few parsecs in size; the velocity dispersion in the Cloudlets is only 1 km/sec. Strong temperature variations in the gas are in evidence.


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