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21 - 30 of 916 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 916 match some words.

  1. Results that match 1 of 2 words

  2. Index of /~vasily/sdss/ngc2419

    https://people.ast.cam.ac.uk/~vasily/sdss/ngc2419/
    2013-08-20 15:07. -.

  3. 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

  4. Index of /~vasily/sdss/spectra

    https://people.ast.cam.ac.uk/~vasily/sdss/spectra/
    2006-05-04 20:41. -. 2007-02-14 14:55. -. 2007-10-15 14:44. -.

  5. Index of /~vasily/sdss/dots

    https://people.ast.cam.ac.uk/~vasily/sdss/dots/
    Index of /vasily/sdss/dots. 2009-01-29 12:15. -. 2009-01-29 12:15. 8.8K. 2009-01-29 12:15. 7.7K. 2009-01-29 12:15. 47K. 2009-01-29 12:15. 3.0K. 2009-01-29 12:15. 2.7K. 2009-01-29 12:15. 5.7K. 2009-01-29 12:15. 28K. 2009-01-29 12:15. 8.7K. 2009-01-29

  6. Index of /~wfcam/docs/reports

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/
    10 18:48. -. 2006-01-17 10:49. -. 2004-05-20 14:51. 79K.

  7. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html
    3 Sep 2007: Passband. Measured 5-sigma limiting magnitude. Magnitude at 50% completeness. Z. 20.8. ... Software. 5-sigma limiting magnitude. Magnitude at 50% completeness. artdata. 20.00. 19.9.

  8. Index of /~vasily/sdss/leos

    https://people.ast.cam.ac.uk/~vasily/sdss/leos/
    Index of /vasily/sdss/leos. 2009-04-24 20:10. 39K.

  9. Index of /~vasily/sdss/stellar_halo

    https://people.ast.cam.ac.uk/~vasily/sdss/stellar_halo/
    2006-11-20 19:40. 29K. ... 2006-11-20 20:00. 1.0K.

  10. Index of /~wfcam/docs/papers

    https://people.ast.cam.ac.uk/~wfcam/docs/papers/
    2006-07-26 18:20. 1.0M.

  11. 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.

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