Sentence examples for smaller redshift from inspiring English sources
We observe a redshift in the gold peak from 526 to 629 nm and a smaller redshift in the silver peak from 410 to 439 nm.
Reid, B. A., Seo, H.-J., Leauthaud, A., Tinker, J. L. & White, M. A 2.5% measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies.
I will discuss the observational and theoretical challenges in measuring and modeling the small-scale redshift space clustering of galaxies in SDSS-III BOSS, as well as its great promise -- we infer the growth rate of cosmic structure at z=0.57 to 2.5% precision and robustly predict the impact of "galaxy" physics on clustering in the quasi-linear regime.
The small redshift of 2D band and the indiscernible D band demonstrated that the tensile strains of up to 40% only induced a strain variation of less than 0.2% and did not cause any observable damage in the graphene film.
From Fig. 6b, we see that P1 almost does not move despite a small redshift at −6%.
The small redshift in the silver absorbance peak is most likely due to an increased size of the core during the formation of the gold shell [17].
The small redshift observed in our samples may be due to the combined effect of bandgap shift with increasing temperature and carrier redistribution among different QDs.
The UV emission peak of the Cu-doped samples showed a small redshift (approximately 6 nm) relative to the undoped ZnO, where the shift is clearer for the samples doped with Cu(NO3) (S4 and S5).
As we looked tangent to the shell, we would see many nearby galaxies with small redshifts.
Matter density perturbations in these models are enhanced at small redshifts because of the presence of a coupling Q that characterizes the strength between dark energy and non-relativistic matter.
Similarly, small redshifts and blueshifts detected in the spectroscopic measurements of individual stars are one way astronomers have been able to diagnose and measure the presence and characteristics of planetary systems around other stars and have even made very detailed differential measurements of redshifts during planetary transits to determine precise orbital parameters.
