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19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the

14 Dec 2006: 2004), we estimate for the firsttime the detection rate of cold debris disks around field M-dwarfs with ages between 20 and 200 Myr. ... al. 2005), the Castor moving group(200 Myr), the Ursa Maj moving group (500 100 Myr asrevised by King et al.

19 Apr 2006: higher surface brightness at r >200 AU compared to the r4 power law. ... but has slightlyhigher surface brightness at r > 200 AU compared to ther4 power law.

28 Sep 2006: event that observations of a secondary photometric standard field with a density of 100-200 objects per detector are available, then the illumination correction can be measured by looking at the

19 Apr 2006: 1984). This excess emission comes from dust in orbitaround the stars and its relatively cold temperature implies thatit resides at large distances from the stars, 30–200 AU, some-thing which ... 2003a) and IRAS observations at 60 and 100 µmhad 3σ

2 Nov 2006: belt width isdr = 0.5r; planetesimal strength is Q?D = 200 J kg. ... kg m3, e = 0.05, e/I = 1,Q?D = 200 J kg.

19 Apr 2006: ac-count and 200 dust particles were produced with exactlythe same positions and velocities as the parent popula-tion. ... for the librationparameters to be fitted for each particle, and the meanparameters for each population of 200 dust grains to

28 Sep 2006: Data Flow System Document Title: VISTA Data Reduction Library Design Document Number: VIS-SPE-IOA-20000-0010 Issue: 1.5 Date: 2006-09-28 Document Prepared by:. Jim Lewis Peter Bunclark Simon Hodgkin (CASU). Signature and Date:. Document Approved by:.

19 Apr 2006: Fitting a Gaussian to therebinned 850 m data indicates that the 850 m emission has aFWHM of 19B4 0B2 and is centered on the star to within 200. ... the disk around star Fomalhaut, which has anage of 200 Myr (Wyatt & Dent 2002).

19 Apr 2006: 20. -10. 0. 10. 20. Dec. off. set,. arcs. ec. É6 200 100 0 -100 -200RA offset, AU. ... 200. -100. 0. 100. 200. Dec. off. set,. AU. Î: Ì î Ï?Ð «0£sU6¤0 09¢&£¤¢?_M«XÓ¢ 9ªsM«ºs¤Ò_Ü£MX?ß 6_ºs_ºs_¡Çà Í