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1 - 10 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. 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.

  3. 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.

  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. 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.

  6. 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

  7. 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

  8. Persistence

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

  9. Persistence Examples

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/persistence/persistence_examples.html
    26 May 2006: m. 20.3. s. 48 31' 40" and has a 2MASS J magnitude of 8.79. ... The individual frames are 20 second exposures taken in Z. About 20 seconds elapse from the end of 01867 and the start of 01868.

  10. Astrometric and Photometric Distortion for WFCAM and VISTA

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

  11. CASU analysis of WFCAM commissioning data - I

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

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