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10 Dec 2012: 2005; Beichman et al. 2006; Brydenet al. 2009), the James Clerk Maxwell Telescope (Hollandet al.

19 Apr 2006: The 850 µm map of Vega obtained by Holland et al.(1998) with the Submillimeter Common-User Bolome-ter Array (SCUBA) on the James Clerk Maxwell Tele-scope shows an extended,

27 Mar 2023: ar 2. 023. 2 M. Booth et al. Bolometer Array (SCUBA) image of the disc taken at theJames Clerk Maxwell Telescope (JCMT) (Greaves et al.1998), there have been claims of

19 Apr 2006: 1.Recently the structure of the disc was mapped at both 450 and850 µm using SCUBA at the James Clerk Maxwell Telescope(JCMT) (Holland et al. ... We usethe optical constants for each of the components taken from Li &Greenberg (1997, 1998) and compute

5 May 2017: 1991). With the introduc-tion of the Submillimetre Common-User Bolometer Array(SCUBA) to the James Clerk Maxwell Telescope (JCMT),Greaves et al.

5 May 2017: 2 (SCUBA2) installedin the James Clerk Maxwell Telescope (JCMT), thus, incorporatinginformation from small and large angular scale structure.

19 Apr 2006: RESONANT TRAPPING OF PLANETESIMALS BY PLANET MIGRATION: DEBRIS DISK CLUMPSAND VEGA’S SIMILARITY TO THE SOLAR SYSTEM. M. C. WyattUK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, UK; wyatt@roe.ac.uk. Received 2003 June 11;

24 May 2022: Sasha Hinkley ,1 Aarynn L. Carter ,2 Shrishmoy Ray ,1 Andrew Skemer,2 Beth Biller,3 Elodie Choquet,4 Maxwell A.

5 Jul 2011: 1999) using Maxwell-Garnetteffective medium theory. The optical properties of the grains werecalculated using Mie theory, Rayleigh-Gans theory and GeometricOptics in the appropriate size regimes (Bohren & Huffman 1983).This composition

16 Jun 2015: Recently,a dust halo was also detected in far-IR resolvedHerschelandJCMT (James Clerk Maxwell Telescope) images by Matthews etal.