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26 May 2006: The variation measured from faint to bright perturbing star was about 20 counts in the level of the persistent image. ... This indicates that the simple model would only be accurate at the 10-20 counts level.

26 Jul 2006: Last modified: Wed Jul 26 20:32:26 2006.

17 Mar 2006: of 20,000 degree decreases by around 10% for the J/K part. ... 90secs in J/K. UKIDSS LAS Survey ---------------- Median limits(5sigma in 2arcsec aperture) Vega Ks 18.2 H 18.8 J 19.6 Y 20.2.

28 Sep 2006: World Coordinate Systems and FITS Headers. After a mere 20 years the FITS community finally agreed upon a standard way of defining a World Coordinate System (WCS) for telescopes with focal

26 May 2006: scheme.. Dafydd Wyn Evans (dwe @ ast.cam.ac.uk). Last modified: Wed Apr 28 16:20:53 2004.

5 Dec 2006: products and archive 14:00 Photometric Calibration (Jones/Hodgkin) 14:20 Astrometric Calibration (Bunclark/Lewis/Irwin) 14:40 Pipeline processing I(including demo) (Lewis/Irwin) 15:20 Tea 15:40 Pipeline

26 May 2006: The variation measured from faint to bright perturbing star was about 20 counts in the level of the persistent image. ... This indicates that the simple model would only be accurate at the 10-20 counts level.

28 Sep 2006: World Coordinate Systems and FITS Headers. After a mere 20 years the FITS community finally agreed upon a standard way of defining a World Coordinate System (WCS) for telescopes with focal

17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range.

26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation).

31 Jul 2006: 2 Tbyte ingest buffer. 10 Tbytes of raw. 20 Tbytes of processed.

8 Dec 2006: 10. VIRCAM_IMG_FLAT255_0049. 15. VIRCAM_IMG_FLAT255_0050. 10. VIRCAM_IMG_FLAT255_0051. 20. VIRCAM_IMG_FLAT255_0052. 10. VIRCAM_IMG_FLAT255_0053. 25.

8 Dec 2006: 10. VIRCAM_IMG_FLAT255_0049. 15. VIRCAM_IMG_FLAT255_0050. 10. VIRCAM_IMG_FLAT255_0051. 20. VIRCAM_IMG_FLAT255_0052. 10. VIRCAM_IMG_FLAT255_0053. 25.

29 Sep 2006: increase the data processing time by approximately 10 to 20%. ... The detailed processing time of this test is:. recipe time = 320 seconds ( 20% for missing functionalities).

2 Nov 2006: The above plots are all in the WFCAM instrumental system and the 5-sigma limiting magnitudes for stellar objects in this data in this system are approximately Y = 20.9, J = ... 20.6, H = 19.8, K = 19.1 ,all in a Vega system.

19 Apr 2006: Thirty-two frames with 20 s integration times each were ob-tained for 55 Cnc. ... We azimuthally smoothed this PSF byrotating the image in 20 increments and median-combiningthe resulting frames.

19 Apr 2006: They used this result to explain the inner hole in the  Pictoris disk by a planet at 20 AU:. ... 850 m : 320 m – 20 cm. Since the size cut-off for resonance is 300 m – 2 mm, I predict:.

19 Apr 2006: than 20 per cent for stars with twice the metal content of theSun (Fischer & Valenti 2005; Santos et al. ... HD 13445 (K1V) 0.20 HD 10700 (G8V) 0.36HD 143761 (G0V) 0.14 HD 196378 (F7V) 0.32HD 192263 (K2V) 0.07 HD 20794 (G8V) 0.23HD 117176 (G5V)

19 Apr 2006: Large-scale mapping of the central 5 pc of the Galaxy at10, 20, and 30 lm at 400 angular resolution by Telesco et al.(1996) found a temperature gradient consistent with ... We estimate a uni-form ISM across our 11.7 and 18.2 lm passbands of 2.86and 2.20,

5 Oct 2006: whole southern celestial hemisphere (20,000deg2) to a depth 4 magnitudes fainterthan 2MASS/DENIS in at least two wavebands J and K.