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{\bf WFCAM Catalogues}
https://people.ast.cam.ac.uk/~wfcam/docs/catalogues.html4 Feb 2006: 19 Error in pkht. 20 Aperture flux 1 These are a series of different radii soft-edged apertures designed to. ... 26 Aperture flux 4. 27 Error in flux Starting with parameter 20 the radii are:. -
WFAU Tapes === Store 6 x dual PCs 3GHz ...
https://people.ast.cam.ac.uk/~wfcam/talks/ukirt_may2006.ppt31 Jul 2006: 2 Tbyte ingest buffer. 10 Tbytes of raw. 20 Tbytes of processed. -
Flat Exposure Properties of VIRCAM Detectors
https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/vircam_flatreport.html8 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. -
Estimate of the Number of CPU Nodes to Execute ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf29 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). -
CASU analysis of WFCAM commissioning data - I
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/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. -
L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...
https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf19 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. -
Basic Debris Disk Model
https://people.ast.cam.ac.uk/~wyatt/wyatt_tpf_jul04.ppt19 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:. -
mnr9848.tex
https://people.ast.cam.ac.uk/~wyatt/gfw05.pdf19 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) -
LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...
https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf19 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, -
, EUROPEAN SOUTHERN OBSERVATORY Organisation Européenne pour des…
https://people.ast.cam.ac.uk/~rgm/vhs/eso-p79b-vhs.pdf5 Oct 2006: whole southern celestial hemisphere (20,000deg2) to a depth 4 magnitudes fainterthan 2MASS/DENIS in at least two wavebands J and K.
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