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19 Apr 2006: A&A 433, 1007–1012 (2005)DOI: 10.1051/0004-6361:20042073c ESO 2005. Astronomy&. Astrophysics. The insignificance of P-R drag in detectableextrasolar planetesimal belts. M. C. Wyatt. UK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9

28 Nov 2006: a Significance of 24 m excess (eq. [1]).b Significance of 70 m excess (eq. ... 2000). Finally,HD 23249 and HD 55892 have 2 < 24 < 3 and 70 < 2.

16 Nov 2006: 2.46 Diopside (CaMgSi2O6) 0.05 3.3 216 0.075 340 1.53 Carbonates Magnesite (MgCO3) 0.07 3.1 84 0.24 370 1.54 Dolomite (CaMgC2O6) d ... 12 and 25 um photometry (Mannings and Barlow 1998), and Spitzer 24 and 70 um photometry.

6 Nov 2006: The UK VDFS review was held on 24/25 October at Cambridge.

19 Apr 2006: Surprisingly, however, the 24 and 70 µm images of Vegaactually have larger radii than the submillimeter ring or mil-limeter clumps (Su et al., 2005). ... Emission (Additional)Vega A0 200 >90 23,24,25 Eridani K2 <1000 60 26,27η Corvi F2 1000 100 28τ

19 Apr 2006: The total measured flux was 1:51 0:24 Jy (S=N 7);the dominant uncertainty in this flux estimate is the calibrationuncertainty.

19 Apr 2006: d)Logarithmic 18.2 km levels : 8.0, 10.6, 13.9, 18.4, 24.3, 32.1, 42.3, 55.9, and 73.7.

15 Apr 2006: B440022.122.24.82.6. V550021.321.49.63.5. R600020.420.817.93.9. I750019.520.035.25.2. Z890018.218.7117.26.3. J12,50016.016.9609.39.3.

19 Apr 2006: 2/)C"C$ )!1-N. 2#1 D 4'@! 24"BC #" 1 9 #"S243! S'@ #3<TU,3- #"D32#!24"24,! :<')("!-! ... $-"8 =H0,"80 N,'<Q ; 3j Y-. ) ,"8 2MP 24 3j ;2)!

2 Nov 2006: 0.5M2v2rel = M1Q? D whereas DD03 define S to be the specific bind-ing energy of the two objects (giving their equation 24). ... dNc(D > Dpb)/dt = 1000r13/3(dr/r)t2ageDcD. 3pb. M4/3? Q? D. 5/6e5/3, (24).

19 Apr 2006: 32 0.02 0.13 0.04 < 0.5HD207129 0.60 0.03 0.15 0.02 0.31 0.04 < 0.24. ... However, sub-mm observations made withSCUBA on the JCMT indicate a diameter of 24 3 arc-sec (Holland et al.

19 Apr 2006: Crosses show the location of a planetesimal in the different resonances (2 : 1, 5 : 3, 3 : 2, and 4 : 3,from top to bottom) at intervals of 1/24 of the ... l1:24. e0:42. ; ð33Þ. D5 :3h i 13:2 þ 290:0=l1:33. ; ð34Þ.

28 Sep 2006: 4.162 2.130 5.626 2.349 -0.529 -0.117 -0.293 0.074 0.105 24.4 2 8.5 283 3.57. ... 4.190 0.301 2.457 1.409 -0.147 0.092 -0.288 0.074 0.132 14.6 10 8.0 859 4.24.

19 Apr 2006: 25 1.24 0.6 IRAS60 9.80 0.62 IRAS60 7.51 0.92 ISO80 8.86 0.87 ISO100 10.95 0.66 IRAS100 11.04 2.0 ISO120

28 Sep 2006: 35 K multiple 20.8. J multiple 24.8UDS 0.77 H multiple 23.8. ... SFA 04:30,25:00 ZY JHK cen. 24. Orion SFA 05:29,02:36 ZY JHK cen.

19 Apr 2006: e5pr. [(a/a2)2.5e/(1 [ e2)1@2 [2.5ae/a2 ] O(e2) , (24). where AU2 yr1. ... P-R draga 6.24 ] 104(M/M. _)b. does not change the plane of the particleÏs orbit, I0pr.

29 Sep 2006: MAGZPT = 24.16 / Photometric ZP (mags) for default extinction. MAGZRR = 0.01 / Photometric ZP error (mags). ... ELLIPTIC= 0.2457458 / Ellipticity estimate from IMCORE. MAGZPT = 24.16 / Photometric ZP (mags) for default extinction.

19 Apr 2006: FX 4V = $= ,d$4 o 24 V4 3 LB44 o -%3-[ 4-C T #"B4V-,d$4 EWVFX -- 44-,"ng$ #"B4V-,d$4E E@$dX 3 ,,3 3V o V234 4 LM,> o ... 3-[ 43 VT #"-_$3-_$ EWVFX ,- 34 #"-_$3-_$E 3FX =., 3 44 o 24 -% $= f 33 o 4-[ --C $FT #"%4 V EW= VFX ,,, 3=4"ng$ #"%4 VE 3FX

28 Sep 2006: 18 5 General Requirements.19 6 Astrometric Requirements. 24 7 Photometric Requirements.25 8 Tiling, Stacking, Microstepping. ... Date: 05/07/2005 Issue: 3.0 Page: Page 24 of 33 Author: W.

28 Sep 2006: 22 4.4 Dome flats. 23 4.5 Detector Noise. 24 4.6 Linearization Measurements. ... 24 4.7 Twilight Flats. 25 4.8 Illumination Correction Measurement. 26 4.9 Image Persistence Measurements.