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6 Jun 2006: The proposed VHS survey will have a 10σ limit in Y of 20.4[Vega]; see Table 1. ... UKIDSS LAS uses SDSS z’ with a median 5σ limit(Vega) of 20.3.

6 Jan 2006: We analyse photometry of the UKIRT faint standardsmeasured on 20 photometric nights.

19 Apr 2006: B-! &-. n u= K G %'. Í 20 10 0 -10 -20RA offset, arcsec. ... $9]! ;9:<8 - P7-& (;! (<$ra A ;{' <9];& C#20% '-&- P (--##; 0B#-3 3;,x,- )/5[?

19 Apr 2006: b) Logarithmic10.8 km levels : 1.3, 1.9, 2.8, 4.2, 6.2, 9.2, 13.7, 20.2, 29.9, 44.3, and 65.5. ... The residual emission (observed minus model ; Fig.4d) at 20 AU from the star is typically 0.2 times that of(0A.3)the lobes.

19 Apr 2006: from the disk at 160 µm (within the 1-σ contour) is 4Jy 20%. ... At 20 Å, the heating timescale has lengthenedso that larger temperature fluctuations are observed andthe temperature distribution of the grain has a significanthot tail.

19 Apr 2006: In the two older systems, BD 20 307and HD 69830, this excess is almost entirely silicate emis-sion from small grains. ... statistics suggest a cold debris disk fre-quency of 10–20 % surrounding sun–like stars with a weakdependence on stellar age (Fig.

19 Apr 2006: 103 3 20 10 6HD109573 HR4796 A0V 67 0.005 4 8 2 9. ... HD141569 0.0 10.3 2.0 55.0 2.30.5 0.0 20.1 1.9 84 40.9 0.0 99.5 2.4 114 50.5

28 Sep 2006: 1868 K 3 19.0300 H2 3. Z 1 20.4Y 1 20.3. ... centre with aFWHM of 20′′, and truncated at a maximum offset of 2′.

2 Nov 2006: expect for a belt of a given age, given its radial loca-tion (equations 15-20). ... 3 Substituting in these nominal val-ues into equation (20) and approximating M? =

19 Apr 2006: Arc. seco. nds. 20 0 -20R.A. offset, arcsec. -20. 0. 20.

28 Nov 2006: Typicaldistances range from 10 to 20 pc, closer for M and K stars andfarther for earlier spectral types. ... Stellar fluxes are measured within an aperture of 10 pixels(=1200), with a background annulus from 10 to 20 pixels.

19 Apr 2006: 95.3 0.20 0.01 - 0.032.5 300 95.3 0.12 0.005 - 0.03. ... Since just 5% of the sub-mm emissioncomes from grains either < 300 µm or > 20 cm in diam-eter, with roughly equal weightings in this range towarddifferent.

28 Sep 2006: 3.238 1.000 4.193 1.548 -1.018 0.194 -0.272 0.073 0.110 20.0 2 8.0 386 3.53. ... 5.172 0.640 3.379 1.475 -0.390 -0.367 -0.293 0.076 0.132 16.3 20 9.0 686 4.66.

19 Apr 2006: 1.41 210 20 1.0 0.2 1.84 0.02 0.20 0.08 0.042 : 1. ... 20. No. significant correlation could be found of D with either l orh for any of the resonances.

19 Apr 2006: ii) Collisional lifetimearguments imply that the collisional cascade starts with planetesimals 1.5–4 km in diameter,and so has a mass of 20–30 M. ... a 125-au radius ring inclined at 20 to the line of sight.

18 Jul 2006: The total archive is about 20-25 Tbytes in size and has been backed up onto tape (100 Ultrium LTO-II tapes). ... These will be further discussed at the VISAS meeting in Edinburgh (20/21 June) which JRL will be attending to represent CASU.

19 Apr 2006: 1). For example, Fig. 2 shows the complex ec-centricities of planetesimals that are at a = 1.4, 1.45 and 1.5aplat 20 equal timesteps ending at a time of ... Assuming the planet wasintroduced when the star (of mass 2.5 M) was born 5 Myr ago,this gives a

29 Sep 2006: 20 Aperture flux 1 Aperture_flux_1 ADU. 21 Aperture flux 1 error Aperture_flux_1_error ADU. ... TUNIT40 = ’ADU ’ / physical unit of field. VDF-WFA-VSA-004, Draft 1.0, September 2006 20.

19 Apr 2006: 8 G'4-5:20"&. / -$>= JLKNKMK. '," ;"8 0 "8 2(4 / 18! ... 838 Y=,"9))-/g" ,R35! 4$6 0 Y "& 3! 4" >2)! - B" 20"!

29 Sep 2006: 18 4.3 Triage. 19 4.4 Software. 20 4.5 Hardware. 21. 4.5.1 Processing Power. ... Doc: VIS-SPE-IOA-20000-0017 Issue: 1.0 Date: 2006-09-28. VISTA Data Flow. System. Cambridge Reduction and Analysis Pipeline Page: 20 of 23.