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https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf19 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. -
Oxford Meeting
https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt15 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. -
Mon. Not. R. Astron. Soc. 334, 589–607 (2002) Collisional ...
https://people.ast.cam.ac.uk/~wyatt/wd02.pdf19 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 -
arX iv:a stro -ph/ 0601 592 v1 26 J ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/hewettetal.pdf28 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. -
THE ASTROPHYSICAL JOURNAL, 527 : 918È944, 1999 December 20The ...
https://people.ast.cam.ac.uk/~wyatt/wdtf99.pdf19 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. -
arX iv:a stro -ph/ 0603 608 v2 1 Se ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/dye.pdf28 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. -
��������� �� ��� ������� ������������������������� � � �!� � ...
https://people.ast.cam.ac.uk/~wyatt/wdg03.pdf19 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 -
VDF-WFA-VSA-004-I1.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-WFA-VSA-004-I1.pdf29 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. -
VDFS UK VISTA User Requirements
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-SPE-IOA-00009-0001.pdf28 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. -
Document Title: VISTA Infra Red Camera Calibration Plan Document ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0002.pdf28 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.
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