Search

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.

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.

19 Apr 2006: Dominik,5 and H. J. Walker6. Received 2004 September 17; accepted 2004 December 20; published 2005 January 10. ... The total dust flux within a diameter circle is′1 37.0mJy at 850mm and mJy at 450mm, in good2.5 250 20.