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24 Jan 2018: The picture shows the evolution of a thin representative slice of the universe (4 Mpc/h x 4 Mpc/h comoving) as a function of time (represented as a scale factor a). The evolution starts at z20 (a0.05) and stops at z=4 (a=0.2). The respective panels

5 Jul 2018: 0.43. 20. Deuterium is the baryometer of choice. FIG. 1. Primordial abundances of the light nuclides as a function of cosmic baryon content, as. ... 0.43. 20. Cen. V = 0.61. B1 III. d = 120 pc.

12 Jul 2018: 1/20 q. 3/20. [You may use the result that in this limit.

29 Mar 2018: NEO/Atira Earth-crossing? 20. The Sun and stars distort space-time and the path of light. ... Slide Number 20. Slide Number 21. Slide Number 22. Tracking stardust: origins of the chemical elements.

24 Jan 2018: The hashed region for the simulation delineates the 20 and 80 per centile of bootstrap re-sampled mock samples.

23 Oct 2018: SN Cosmology Project. 14. 16. 18. 20. 22. 24. 0.0 0.2 0.4 0.6 0.8 1.01.0.

31 Jul 2018: In that regard, animportant wavelength regime is the mid-infrared (5-20 µm). ... 17.4 25.0 20.5 35 Suggestion of life CH4 7.37 7.96 7.65 13.

30 Oct 2018: 0.43. 20. Cyburt+ 2015. L Kewley. Aver+ 2015. BBN theory confronts observations 2015.

9 Mar 2018: 160µm. 20 10 0 -10 -20α cos δ offset ("). GJ 3634, nearby sources. ... 100µm -0.20. -0.12. -0.03. 0.05. 0.13. 0.22. 0.30. mJy. arc. sec-.

10 Oct 2018: ȧ2 =8πGρ0. 3. 1. a(2.20). which has the solution a t2/3. ... a(t) =. (t. t0. )2/3; ρ(t) =. ρ0a3. =ρ0t. 20. t2(2.21).

11 Oct 2018: 5. G11 = c2 (2aä ȧ2 k) (1 kr2)1 (3.20). Substituting (3.18), (3.19) and (3.20) into (3.16), we obtain two distinctdynamical relations for the time evolution

30 Jul 2018: This translatesin a 20% increase in yield for an exo-Earth imaging mission of a given size [14]. ... position angle of LBTI’s transmission pattern.Again, a variation of 20% can be expected.

8 Nov 2018: In the last 20 years, the near-exponential increase incomputational power (in both hardware and software) has made it possibleto carry out increasingly sophisticated simulations of large volumes of theUniverse to

30 Jul 2018: 21, 22,. Eq. 17 and Eq. 20. 4 A MODEL FOR THE FATE OF PARTICLES. ... 20, Eq. 17using δa = 1/2 and δe = 5/2, as described in 4.1.

13 Nov 2018: 20. 8πGmH(12.16). (Y is the baryonic mass fraction in He: Yp = 0.24) and. ... bHubble H(z) L/2 km s1 (12.20). where H(z) is the Hubble parameter which, as we know (Lecture 5) isgiven by:.

31 Jul 2018: Each offset is determined byminimizing the RMS scatter in the combined light curves forall observers, operating on 20-day bins. ... We have analyzed this fast light curve for ef-fects that would be averaged over with 20-day binning.

25 Oct 2018: u =g. (2πh̄)3. 0. f(E)E(p) 4πp2 dp (7.20). The distribution function in energy terms, f(E), is given generally by:. ... 3; dp =. kT. cdy. so that eq. 7.20 can be re-written as:.

9 Nov 2018: ys. 30. 20. 10. 0. 10. Figure 1. A segment of the raw and filtered KIC 3542116 light curves (upper panel), and the corresponding test statistic Tn,w (lowerpanel). ... Comparing these numbers to Figure 14 ofWyatt et al. (2018), the improved sensitivity

23 Oct 2018: 9. 14. 16. 18. 20. 22. 24. 0.0 0.2 0.4 0.6 0.8 1.01.0. ... ρi ani , (6.19). where:ni = 3(1 wi). (6.20). Our definition of the density parameter:.

20 Jul 2018: The ubiquity of debrisdisks is apparent from the fact that such circumstellar dust is present at a detectablelevel around 20% of nearby main sequence stars. ... For both spectral types, approximately 20% ofstars have detectable disks (Eiroa et al.