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25 Oct 2018: At t 106 s, T 101213 K' 200 MeV – 1 GeV (the QCD, or Quark-Hadron transition), is when quarks can no longer exist on their own;they combine into hadrons

30 Oct 2018: The relative abun-dances of the light elements created in BBN remained unaltered for thefirst 200 Myr.2 However, once the first stars formed at z 20, theBBN abundances began to

6 Nov 2018: 200 Mpc) from their celestial coordinatesand redshifts. This exercise produces a dipole that is in good agreement, inboth magnitude and direction, with that of the CMB, lending support tothe interpretation of

20 Nov 2018: 2014). 100 150 200 2500. 0.2. 0.4. 0.6. 0.8. 1. r!

22 Nov 2018: Figure 16.1: M31, the Andromeda galaxy, photographed with a Canon 200 mm telephotolens.

5 Jul 2018: N(H I) = 2.5 1020 cm2. Fe/H = 1/200 solar. Very Metal Poor DLAs are the choice astrophysical environments for measuring the primordial abundance of deuterium.

30 Jul 2018: MNRAS 000, 1–23 (2015) Preprint 30 July 2018 Compiled using MNRAS LATEX style file v3.0. Using warm dust to constrain unseen planets. Amy Bonsor1, Mark C. Wyatt1, Quentin Kral1, Grant Kennedy2,3, Andrew. Shannon4,5 and Steve Ertel61Institute of

31 Jul 2018: Approximately 85 planets could be habitable (radii between 0.5 Rand 1.75 R and equilibrium temperatures between 200 K and 450 K) andwould be prime targets for follow-up spectroscopic ... Earth orbiting α Cen and 10 small planets (1 to 4 R) with

2 Apr 2018: arX. iv:1. 803. 1126. 5v1. [as. tro-. ph.S. R]. 29. Mar. 201. 8Draft version April 2, 2018. Typeset using LATEX twocolumn style in AASTeX61. THE HOSTS SURVEY – EXOZODIACAL DUST MEASUREMENTS FOR 30 STARS. Ertel, S.,1 Defrère, D.,2 Hinz, P.,1

30 Jul 2018: 2002). [20] Mérand, A., Bordé, P., and Coudé du Foresto, V., “A catalog of bright calibrator stars for 200-m baselinenear-infrared stellar interferometry,” A&A 433, 1155–1162 (Apr.