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14 Sep 2015: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 14 September 2015 (MN LATEX style file v2.2). Planet Hunters X.KIC 8462852 – Where’s the flux? †. T. S. Boyajian1, D. M. LaCourse2, S. A. Rappaport3,D. Fabrycky4, D. A. Fischer1, D.

16 Jul 2021: The hori-zontal lines separate the (top) Band 6, (middle) 2016 Band 7 and (bottom)2018Band7observation sets.All times represent time on source.

19 Feb 2018: a test of whether an IR excessis present.

12 Apr 2013: Figure 4. Critical Hill semimajor axis ratios as a function of stellarmass for different eccentricities (upper panel), different mutual incli-nations (middle panel) and different planetary masses (bottom panel).The purple

23 Nov 2021: While ALMAclearly shows dust concentrations (e.g. van der Marelet al., 2013; Casassus et al., 2013), we cannot test ourunderstanding of radial migration, settling, and graingrowth without quantifying the gas reservoir

24 Oct 2015: the star-forming gas reservoirs within and beyond the CND(e.g., Liu et al., 2012)—such as peculiar objects like the G2 cloud (Gillessenet al., 2012)—to test scenarios of ... FIG. 3.ÈNatural weight VLA maps of the sources VLA 1 and 2, made with the 6

7 Nov 2016: tance to the star along the major (top panel) and minor axis ofthe disc (middle panel) obtained averaging over 40 wide wedges.In the bottom panel we present the mean intensity ... In order to test the latter scenario andsee if the disc morphology can be

23 Mar 2007: 2005), F24disk/F24? 150t1age ,is shown with a solid line. (Middle) Fraction of stars with fluxratios in the different age bins used by Rieke et al.

18 Oct 2014: A Fisher’s exact test shows that there is only. a 0.7% chance of detecting rates as discrepant if the two groups had the same distribution.

23 Jan 2014: While Figs 2b and 2d provide the best estimate of theunderlying inferred accretion rate distributions in the sub-samples, we will also use Fisher’s exact test to assign a