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1 - 10 of 68 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 68 match some words.

  1. Results that match 1 of 2 words

  2. Persistence

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

  3. Richard McMahon, Institute of Astronomy, Cambridge University:…

    https://people.ast.cam.ac.uk/~rgm/presentations/
    26 Jul 2006: Last modified: Wed Jul 26 20:32:26 2006.

  4. https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt

    https://people.ast.cam.ac.uk/~rgm/vhs/vhs-baseline-v3.txt
    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.

  5. Astrometric and Photometric Distortion for WFCAM and VISTA

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

  6. CASU WFCAM/VISTA Explanation of documentation numbering system>

    https://people.ast.cam.ac.uk/~wfcam/docs_exp.html
    26 May 2006: scheme.. Dafydd Wyn Evans (dwe @ ast.cam.ac.uk). Last modified: Wed Apr 28 16:20:53 2004.

  7. Contents

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/index.html
    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.

  8. https://people.ast.cam.ac.uk/~rgm/wfcsur/meetings/announcement_2.txt

    https://people.ast.cam.ac.uk/~rgm/wfcsur/meetings/announcement_2.txt
    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

  9. 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:.

  10. 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)

  11. 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,

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