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19 Apr 2006: The new dust libration parameters were thenused to work out the spatial distribution of these grains. ... The new centrecan be derived by making the sum of the inward decaydue to P-R drag (eq.

14 Dec 2006: We have detected a new debris disk around the M0.5 dwarf GJ 842.2 at λ = 850 µm, providing evidence for cold dust at largedistance from this star (300 AU). ... 2005). Ourcontribution to establishing the statistics of debris disks aroundM-dwarfs

19 Apr 2006: A&A 440, 937–948 (2005)DOI: 10.1051/0004-6361:20053391c ESO 2005. Astronomy&. Astrophysics. Spiral structure when setting up pericentre glow: possible giantplanets at hundreds of AU in the HD 141569 disk. M. C. Wyatt. UK Astronomy Technology Centre

19 Apr 2006: to theobservations of debris disks around other stars; and e) how these new results impactour assessment of whether systems like our own are common or rare compared to theensemble of normal ... Several new far–infrared studies were initiated with

29 Sep 2006: a tile, input pawprints will have to be resampled onto a new grid. ... 3 3 9. 2 IOA MJI New Hire Recruitment delays Personnel Temporary reassignment.

28 Sep 2006: For these reasons a new Z-band filterhas been designed for use with WFCAM. ... The same philosophy wasadopted in the design of the new Z and Y filters.

19 Apr 2006: Mon. Not. R. Astron. Soc. 334, 589–607 (2002). Collisional processes in extrasolar planetesimal discs – dust clumpsin Fomalhaut’s debris disc. M. C. Wyatt and W. R. F. DentUK Astronomy Technology Centre, Royal Observatory, Blackford Hill,

28 Sep 2006: Notification List The following shall be notified when a new version of this document is issued Exeter Tim Naylor ATC Malcolm Stewart. ... Movement: A change of position of the telescope that is not large enough to require a new guide star.

29 Sep 2006: WCSPASS = 2. RAZP02 = 10.09369 / [arcsec] Ref RA shift pass 0 to 2 (new - old). ... DECZP02 = -1.578503 / [arcsec] Ref Dec shift pass 0 to 2 (new - old).

19 Apr 2006: 1. INTRODUCTION. A new generation of astronomical instrumentations isnow making it possible to image the thermal emission fromthe disks of dust that surround some stars.

28 Sep 2006: 2006).The design involves a new f /9 secondary, which producesan intermediate focus 5.7m above the primary.

28 Sep 2006: Plan Page: 3 of 71. Notification List The following people should be notified by email that a new issue of this document is available. ... Movement A change of position of the telescope that is not large enough to require a new guide star.

28 Sep 2006: Notification List The following people should be notified by email that a new issue of this document is available. ... Preset A telescope slew to a new position requiring a reconfiguration of various telescope systems.