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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

2 Jan 2018: take. )C. /200. 1 A. 2 (L. INEA. R). C/2. 012.

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

19 Feb 2018: With the exception of HD166, with an age of 200 Myr, these five bright discs are all fairlyold systems, with a mean age of 2.5 Gyr.

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.

31 Jul 2018: 4.1 Planet mass and semi-major axis distribution. We consider a chain of planets on circular co-planar orbits,with masses varying from 1 to 200 M (0.63 MJup) ... Inorder to minimise random effects caused by the finite num-ber of particles used in these

23 Aug 2018: MNRAS 000, 1–13 (2018) Preprint 23 August 2018 Compiled using MNRAS LATEX style file v3.0. Fast spectrophotometry of WD 1145017. Paula Izquierdo1,2?, Pablo Rodŕıguez-Gil1,2, Boris T. Gänsicke3,4, Alexander J. Mustill5,Odette Toloza3,

31 Jul 2018: year for the first thousanddays (for a drop of 0.9%), then a fast drop by 2% over 200days, followed by a slow decline for the last 200 days (Montet& Simon ... that wouldhave a duration of perhaps 200 years.

5 Apr 2018: HD 8907 34.8 F8 2.0 1.2 200 80.0 52.0 46.5 2.3e-04 1. ... HD 107146 27.5 G2V 1.0 1.0 200 88.6 126.8 37.8 8.6e-04 9.

20 Jul 2018: Fig. 3 Observations of the debris disk of the 80-200 Myr G2V star HD107146 (Marino et al., inprep.).

14 Jun 2018: 2017 The Authors. 2 M. C. Wyatt et al. 200 400 600 800 1000 1200 1400 1600Time (BJD-2454833). ... min(rt)/R? = (π/4)min(δobs)/max(fobs) 200, (16). Figure 4. Geometrical quantities that translate into observables.

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: MNRAS 479, 2649–2672 (2018) doi:10.1093/mnras/sty1677Advance Access publication 2018 June 26. Cometary impactors on the TRAPPIST-1 planets can destroy all planetaryatmospheres and rebuild secondary atmospheres on planets f, g, and h. Quentin