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DWE's Gallery
https://people.ast.cam.ac.uk/~dwe/gallery/18 May 2018: You paint this onto glass, let it dry for 24 hours and bake it in the oven at 160C. -
Gaia DFS PLS prop
https://people.ast.cam.ac.uk/~gil/Gaia-RAeS-Leslie-Bedford-April2017.pdf29 Mar 2018: Slide Number 24. Gaia science: learning how to learn. Slide Number 26. -
Astronomy and Astrophysics in the Gaia skyProceedings IAU Symposium…
https://people.ast.cam.ac.uk/~gil/gaia_from_proposal_to_gdr1.pdf26 Mar 2018: 24 G. Gilmore. Figure 1. The ROEMER proposal to ESA in 1993. -
M. Pettini: Introduction to Cosmology — Lecture 1 BASIC ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture01.pdf8 Oct 2018: In cgs units:. H0 = 3.24 1018h s1 (1.11). Clearly, the time for a galaxy at a distance d, moving at velocity v, to moveapart by a further distance d -
M. Pettini: Introduction to Cosmology — Lecture 2 NEWTONIAN ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture02.pdf10 Oct 2018: ρ 1a4. (2.23). 7. and. a(t) =. (t. t0. )1/2; ρ(t) =. ρ0a4. =ρ0t. 20. t2(2.24). This is the second classic cosmological solution. -
M. Pettini: Introduction to Cosmology — Lecture 3 RELATIVISTIC ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture03.pdf11 Oct 2018: 2.12), the Friedmann equation (3.21) takes theform:. ȧ20 =8π. 3Ga20ρ0 kc2 = H20a200 kc2 (3.24). -
M. Pettini: Introduction to Cosmology — Lecture 5 REDSHIFTS ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture05.pdf18 Oct 2018: 2.21 and 2.24). Thus,we do have a horizon. We also recall (from eq. ... 2.24). With this func-tional form, we find that in the radiation dominated era, the horizon scalewas. -
M. Pettini: Introduction to Cosmology — Lecture 6 THE ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture06.pdf23 Oct 2018: 9. 14. 16. 18. 20. 22. 24. 0.0 0.2 0.4 0.6 0.8 1.01.0. ... ρk = 3. 8πG. k. a2(6.24). which varies as ρk a2, so that for curvature w = 1/3. -
Introduction to Cosmology Lecture 6 Loveday+ 2012 Reddy & ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture06_slides.pdf23 Oct 2018: SN Cosmology Project. 14. 16. 18. 20. 22. 24. 0.0 0.2 0.4 0.6 0.8 1.01.0. -
M. Pettini: Introduction to Cosmology — Lecture 7 THERMAL ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture07.pdf25 Oct 2018: We also saw in Lecture 2 (eq. 2.24) that in the radiation-dominated era thescale factor of the Universe evolves as a(t) = (t/t0). ... 7. 8. g. 2aT 4 for fermions,. (7.24). in equilibrium when kT mc2.
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