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9 Nov 2018: In total the datacomprise four years of photometry for roughly 200,000 dis-tinct stars.

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

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.

31 Jul 2018: Only HD 107146, an 80 200 Myr old G2V star(Williams et al. ... disc. In fact, the visibilities ofthe inner component are negligible beyond 200 kλ.

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

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

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

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

22 Nov 2018: 10 correspond tothe locations and radial velocities at which gas is expectedto emit if on a circular orbit at 40 and 200 au (assuming a1.77 M star, Moór et al. ... 2015). The PV-diagram thus tellsus that the bulk of the gas disc is between 40 and 200

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