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11 - 20 of 74 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 74 match some words.

  1. Results that match 1 of 2 words

  2. {\bf WFCAM Catalogues}

    https://people.ast.cam.ac.uk/~wfcam/docs/catalogues.html
    4 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:.

  3. WFAU Tapes === Store 6 x dual PCs 3GHz ...

    https://people.ast.cam.ac.uk/~wfcam/talks/ukirt_may2006.ppt
    31 Jul 2006: 2 Tbyte ingest buffer. 10 Tbytes of raw. 20 Tbytes of processed.

  4. Flat Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/vircam_flatreport.html
    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.

  5. Estimate of the Number of CPU Nodes to Execute ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf
    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).

  6. 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.

  7. L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...

    https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf
    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.

  8. Basic Debris Disk Model

    https://people.ast.cam.ac.uk/~wyatt/wyatt_tpf_jul04.ppt
    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:.

  9. mnr9848.tex

    https://people.ast.cam.ac.uk/~wyatt/gfw05.pdf
    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)

  10. LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...

    https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf
    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,

  11. , EUROPEAN SOUTHERN OBSERVATORY Organisation Européenne pour des…

    https://people.ast.cam.ac.uk/~rgm/vhs/eso-p79b-vhs.pdf
    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.

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