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17 May 2016: New York, NY 10034, USA6Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1562, USA7Joint ALMA Observatory, Alonso de CÃşrdova 3107, 763-0355 Vitacura, Santiago, Chile8Exoplanets and Stellar ... al. 2013). After one

27 Jan 2016: This result sets a new record for high-contrast mid-infrared interferometricimaging and opens a new window on the study of planetary systems. ... New alignment. 8 Defrère et al. procedures will be developed during the science valida-tion phase to

23 Sep 2016: As one of the main goals of this work is to directly com-pare this new Band 6 CO J=2-1 dataset with the archivalCO J=3-2 Band 7 ... Finally, inSect. 3.3.3 we carry out a PV diagram comparison betweenthe new CO J=2-1 and the archival J=3-2 dataset.

7 Nov 2016: 1 Described in https://almascience.eso.org/news/notification-. always consistently centered on the star and neither were theoffsets always equal.

15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant

7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot,