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17 Mar 2006: o Legacy value, Serendipity and new classes of object. o Maximising the science return from ESA missions, XMM-Newton, Planck, Herschel and GAIA.

18 Jul 2006: The Panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in JK only.

18 Jul 2006: 6. WFCAM news (Non)linearity saga - this one could run for a long time. ... 7. VDFS news PSB reported that he had a productive visit to RAL and that he has returned with 270 files - all with full headers.

26 Jan 2006: The good news is these artefacts are non-astronomical in appearance and do not "talk" across the detector quadrant boundaries, or between detectors; the bad news is that they do not ... Darks. The darks, including new improved residual reset anomaly now

21 Oct 2006: Progress is being made - ongoing EGS has made the new ING archive interface the default one. ... He also noted that various UKIRT new project Letters of Intent were being circulated to those likely to interested.

2 Aug 2006: Optical processing update 5. WFCAM news - reprocessing 05B - progress with 06A - non-linearity update - MSB ID checksum for tagging bad MSBs 6. ... VISTA news - VIRCAM AIT status and data - VDFS docs status - DRL status 7.

2 Nov 2006: taken roughly in the middle of the night (and as it happens also taken within 4 days of new moon).

18 Jul 2006: Optical processing update 5. WFCAM news 6. VDFS news 7. Plone update 8. ... 6. VDFS news There was not much new news on VIRCAM since WJS was away.

6 Nov 2006: Tests are underway on the new baffling tube which should cut out remaining Moon glint problems. ... New acquisition hardware has been installed and still has a few teething troubles.

1 Oct 2006: WFCAM news 8. VISTA news 9. UK review 10. VISTA public surveys 11. ... DWE reminded ALL about the location of Plone site. A web new server has bought and installed.

11 Mar 2006: News on VISTA survey proposal front: WJS said that he knew of 9 surveys that had been proposed. ... Meanwhile, we were all asked to look at the new site and send in comments to DWE and EGS.

2 Feb 2006: DWE said that this would be sorted out with the new Plone system. ... ETC - This new CASU requirement occupied most of PSB's (& some of MJI's) time during January.

8 Sep 2006: Actions from last meeting 2. Comments on WFAU minutes 3. News from IAU GA 4. ... Optical processing update 8. WFCAM news 9. VISTA news 10. AOB Minutes ------- 1.

18 Apr 2006: New files are checked to see they are in a sensible location and then copied over to the Plone system. ... The new sky processing strategy creates a lot (500/night) of intermediate step sky frames (xskys).

9 Aug 2006: MJI compared old and new versions of the catalogue software and MR also compared toolkit development version with pipeline version. ... This includes new surveys and even new instruments (sic!). The one new survey all present agreed on was the idea of a

31 Jul 2006: V2. fixed stacks, better sky, full standard catalog parameters,. new 2MASS ce’s = EDR version. ... 1 #3 05B cross-talk full standard 2MASS new ce Oct 2005removed parameter set (DR1 version) -Feb 2006.

27 Mar 2006: Actions from last meeting JRL has not received any news about the OMP database mirror and its repair. ... News on science with WFCAM data: STH said that a paper on alpha Sco was in production.

13 Oct 2006: New disks: >30mJy (none), 10-30mJy (5), 3-10mJy (9). • Mean flux of non-detections is 0.3mJy. • ... Expect some structures explained by current models. • For others new dynamical models will be developed.

15 May 2006: A new idea has come up of creating a new Plone state of "obsolete". ... VDFS news VIRCAM Status AITnn: WJS reported on the status of the telescope, mirror, dome and camera.

9 Jan 2006: RGM noted that this was an impressive achievement to start the New Year with. ... UKIRT There is no new data for the UKIRT archive at the moment.

3 Aug 2006: New measures:• MAGZPT• MAGZRR (per frame ‘error’)• NIGHTZPT• NIGHTZRR (per night ‘error’). •

18 Jul 2006: The Panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in JK only.

19 Apr 2006: All rights reserved. Printed in U.S.A. NEW SUBMILLIMETER LIMITS ON DUST IN THE 55 CANCRI PLANETARY SYSTEM. ... 2000), which was already a factor of 100 below. L96 NEW SUBMILLIMETER OBSERVATIONS OF 55 CNC Vol.

21 Oct 2006: The new detector 10 doesn't have this sort of problem nor do any of the others. ... Having this level of redundancy is excellent news if we want to use the data themselves to correct the problem.

5 Oct 2006: If yes, explain why the need for new data. Are the data requested in this proposal on the ESO Archive (http://archive.eso.org)?

19 Apr 2006: Our observations provide new information aboutthe distribution of the color temperature and optical depthstructure of this region. ... The high resolution of mid-infrared detec-tors on new large telescopes, such as Gemini, VLT, and theGTC, will permit

19 Apr 2006: ABSTRACT. New submillimeter images have been obtained of the dust disk around the nearby K2 V stare Eridani, withthe total data set now spanning 5 yr. ... 4. DISCUSSION. The new images of thee Eri dust ring confirm its structureand dimensions, and the

9 Oct 2006: This required a total time of 7359hrs based on VISTA ETC(v1.1).With the new VISTA ETC(v1.3) this reduces to a total of 6750hrs. ... PSP Panel Issue 5 The Panel strongly recommends that the PI submits a new proposal whichfocused on the science that can be

19 Apr 2006: Received 2002 April 17; accepted 2002 September 20. ABSTRACT. New submillimeter images of the cold dust emission around the nearby main-sequence star Fomalhaut arepresented. ... object. 5. CONCLUSIONS. We have presented new, high signal-to-noise ratio sub

19 Apr 2006: Here we present new mid-IR observations of the Vega-likestar HD 141569 (B9.5 Ve).

8 Mar 2006: GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad band background. ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of 0.1 per cent are needed compared with 1%

15 Apr 2006: Infrared OH Sky Observations: Mahaira etal, 1993, PASP. GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of

19 Apr 2006: A new 850-µmimage shows that there is indeed such a debris disc, extending out to 55 au (15 arcsec)radius.

16 Nov 2006: A set of components was tested. exhaustively before the addition of a new species was allowed, and only species that reduced. ... New work by Wyatt et al. (2007) also demonstrates that it is highly unlikely that an asteroid.

19 Apr 2006: 1999). Here we present new 10.8 and 18.2 km images, obtainedat the Keck II telescope, of the HR 4796A debris disk. ... Our new images clarify the structure of the central clear-ing zone, or hole, which may be indirect evidence for aplanet orbiting HR

19 Apr 2006: All rights reserved. Printed in U.S.A. et al. 2004). Since the three newly resolved disks are around Gand M stars, these new images are filling in our understanding ofhow ... TheIRAS fluxes were determined from SCANPI (IRAS Scan Pro-cessing and

19 Apr 2006: Table 1. New observations used in our analysis. Observationsbefore 2000 were extracted from the JCMT archive. ... The top part of the table shows new data, the bottom part showsexisting data.

19 Apr 2006: 2003). An informativeresult from the ISO survey (Habing et al. 2001) was that althoughthe sensitivity was five times greater than for the equivalent searchmade by IRAS, only one new disc was

28 Nov 2006: NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE DIRECT DETECTION OF PLANETS.

6 Jun 2006: 1. Legacy value, serendipity, curiosity and new classes of object, 21st century Infra-Red equivalent of thePalomar-UK-ESO Schmidt Surveys. ... 2. To discover objects cooler than the T-dwarfs and define the new ‘Y’ spectral class.

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.