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31 Jul 2018: Observatory, Carlsbad, California, USA7Bar J Observatory, New Smyrna Beach, Florida, 32168, USA8Angel Peaks Observatory, Cotopaxi, Colorado, 81223, USA9Karen Observatory, 12 Handley Drive, Padgate, Warrington, Cheshire, WA2 0GN, UK10Department of

22 Nov 2018: Extensions of the standard model ofparticle physics known as supersymmetry (SUSY) entertain the existenceof a large number of new particles, the lightest of which would be stable.None have yet been ... Itmust also be said that the supersymmetric WIMP

5 Apr 2018: 0.270.10, where. these new debiased parameters are consistent with the. biased ones. ... The main difference between Fig. 5 and Fig. 3 is. that a new lower envelope of detectability appears at.

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

30 Jul 2018: 2656 Q. Kral et al. Figure 8. New probability map: similar to Fig. ... Figure 9. New ejection map: similar to Fig. 3, but for an inclined distribu-tion of comets (see Section 3.5 for more details).

2 Apr 2018: Our overall detection. rate is 18%, including four new detections, among which are the first three around Sun-like stars and the first two. ... preset to a new star. During the nodding cycles the. beams from both apertures are brought to

19 Feb 2018: 2013)reported a higher rate of 20.2 2 per cent. This result was de-rived from new IR data obtained with the PACS camera (Poglitschet al. ... Five of these sources are identified by Eiroaet al. (2013) as new discs discovered by Herschel.

15 May 2018: spreading material flows beyond the Roche limit, it coagulates into new (mi-nor) planets in a process analogous to the ongoing formation of moonlets at the outer edge ofSaturn’s rings. ... Roche limit is gradually quenched by PRdrag, eventually

14 Jun 2018: MNRAS 000, 1–21 (2017) Preprint 14 June 2018 Compiled using MNRAS LATEX style file v3.0. Modelling the KIC8462852 light curves: compatibility of the dipsand secular dimming with an exocomet interpretation. M. C. Wyatt1?, R. van Lieshout1, G. M.

31 Jul 2018: MNRAS 000, 1–23 (0000) Preprint 6 June 2018 Compiled using MNRAS LATEX style file v3.0. Scattering of exocomets by a planet chain: exozodi levelsand the delivery of cometary material to inner planets. Sebastian Marino1?, Amy Bonsor1, Mark C.