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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.

9 Oct 2006: ESO Public Surveys Proposal Form Phase 1. reaching 10sigma limits[AB mags] in g, r, i and z of 24.1, 23.7, 23.3 and 22.6 respectively. ... with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.

4 Feb 2006: 24 Aperture flux 3 Recommended if a single number is required to represent the flux for ALL. ... 24 arcsec diameter. 45 Error in flux The aperture fluxes can be combined with later-derived aperture.

9 Jan 2006: The last GANTT chart we have says 24 March, but it is unclear if this is the current target date.

9 Aug 2006: 3. Report from VDMT MJI and STH attended the VDMT meeting in Edinburgh on 24 July. ... MJI reported on the main points: The UK review of VDFS will be held in Cambridge on 24/25 October.

1 Oct 2006: JRL volunteered. MJI gave further details of the review. Planned Start 24 October Tuesday 10:30 End 25 October Wednesday 15:30 Lunch will be provided on both days and it ... APM3: We were reminded that the home disks of apm3 have now been united with

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

2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2.

2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2.

26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7.

26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7.

21 Oct 2006: Figure 24 below shows this for detector 15 on the mean dark frame. ... Figure 24 A hot pixel cluster on a mean dark frame for detector 15.

8 Dec 2006: 1.32 /- 0.05. 0.53 /- 0.01. 8. 2.23 /- 0.24. 0.61 /- 0.03. ... figure 5.10 Detector 10 (0.10%). figure 5.11 Detector 11 (0.24%). figure 5.12 Detector 12 (0.22%).

8 Dec 2006: 1.32 /- 0.05. 0.53 /- 0.01. 8. 2.23 /- 0.24. 0.61 /- 0.03. ... figure 5.10 Detector 10 (0.10%). figure 5.11 Detector 11 (0.24%). figure 5.12 Detector 12 (0.22%).

3 Aug 2006: The observations span 05A and 05B, and comprise around 21 obs for the P272 field, and 24 for the P545 field.

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.

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.

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.

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.

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.

28 Sep 2006: 0001, issue 3.2 2005-02-24. [RD 3] VISTA Science Requirements Document, VIS-SPE-VSC-00000-0001, issue. ... 13 / kk leads to a relative area of. )41()31).(1( 222 rkrkrk ′′′ (2-24).

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.

19 Apr 2006: This latter study is based on weak IRAS excesses,and four of the six systems identified with IRAS at 25 µm do nothave 24-µm excesses on re-examination by Spitzer

19 Apr 2006: G8V 1HD 18757 22.9 G4V 2 Wide binaryHD 19373 10.5 G0V 1HD 20407 24.4 G3V 1HD 20766 12.1 G2V 2,‘B’ Wide binary (secondary)HD 20807 ... 1 G1V 2 Wide binary (primary); IRAS discHD 20619 24.7 G5V 1HD 20630 9.2 G5V 1 YoungHD 20794 6.1 G8V 1 ISO discHD

19 Apr 2006: 24(40 AU) in ground-based, near-infrared, coronagraphic images.They estimated the disk position angle as , inclination50 1027 deg, and minimum dust mass 0.4 M. ... Trilling &2. Brown (1998) report an H-band disk surface brightness thatfalls below 24 mag

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.

14 Dec 2006: 2 0.8 0.8 150 20 <1.9GJ 9809 M0 23 06 04.8 63 55 34 24.9 29.43 Loc Ass. ... 23 06 04.8 63 55 34 24.9 29.43 Loc Ass 0.5 7 0.36 2.2 2.2 7 26 <10.

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: MIR.but more common around stars < 100 Myr. MIPS 24 um image of Vega disk. ... MIPS-24 MIPS-70. MIPS-160 JCMT-450CSO-350. HST. Do Stars with Inner Planets (< 5 AU) Also Have Kuiper Disks?

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: 6 Su et al. Fig. 9.— Radial dependent [24][70] distribution for the Vegadisk. ... To produce the observed [24][70]color, additional components must be invoked. 4.4.

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.

19 Apr 2006: Corresponding peak. signal-to-noise ratios are 27, 48, 24 and 15, respectively. ... We used thestandard g Reticulum to determine the PSF at 24.6 mm.

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

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

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.

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.

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: 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.

19 Apr 2006: to the Sun, at about 23 AU, then migratedoutward to its current 30 AU orbit [24]. ... Sci., 27, 287–312 (1999).24. Malhotra, R., Astron. J., 110, 420–429 (1995).25.

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

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)!

27 Jul 2006: Chemical Informatics Letters. Editor:Volume 10. (1). How much does it cost to publish a paper and then have access to the results? This study looks at the library expenditure for universities in the USA, and divides it by the number of articles

27 Jul 2006: Chemical Informatics Letters. Editor:Volume 11. (1). The Senate comment on PubChem. This builds on the earlier decision. The Senate report calls upon NIH to "work with the private sector chemical information providers, with the primary goal of

27 Jul 2006: Some free programs and databases are listed here:. 24).

27 Jul 2006: Chemical Informatics Letters. Editor:Volumes 1-7. Volume 7. (1). FDA: library of chemical information (July 2003). The US Food and Drug Administration now provides a library of chemical information. Isotope Effects Toolkit (July 2003). This web site

27 Jul 2006: Chemical Informatics Letters. Editor:Volume 8. (1). Science Inventory (January 2004). A searchable catalog of more than 4,000 science activities of the US environmental protection agency (EPA). The site allows keyword searches and highlights nine

27 Jul 2006: Chemical Informatics Letters. Editor:Volume 9. (1). Chemical Informatics Letters now available via RSS, which can be viewed on a web browser here, using the RDN's viewer, or by loading. http://www-jmg.ch.cam.ac.uk/CIL/rss/cil.xml. into any RSS reader

14 Jun 2006: This breakdown can be achieved by defining the ‘catchmentbasin’ [23, 24], or ‘basin of attraction’, for each local minimum as the region ofconfiguration space for which steepest-descent paths converge to

8 Mar 2006: It's all there, online, 24 hours a day.”. The ScienceDirect backfiles include such titles as ‘The Lancet’, ‘Physics Reports’, ‘Analytica Clinica Acta’, ‘Topology’, ‘Behaviour Research and Therapy’, ‘Neuroscience’,