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31 - 40 of 909 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 909 match some words.

  1. Results that match 1 of 2 words

  2. 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. -.

  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. 1 Introduction

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf/index.html
    6 Dec 2004: could also be accounted for (the detection limit is about J=20 [Irwin 2003]).

  5. Index of /~xmmssc/xid-imaging/camxid/MBM12

    https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/camxid/MBM12/
    Index of /xmmssc/xid-imaging/camxid/MBM12. 2004-09-13 20:41. 0. ... 2004-09-13 20:32. -.

  6. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_20.pdf
    16 Nov 2017: Structure & Evolution of Stars 1. Structure and Evolution of StarsLecture 20: Supernovae, Core Collapse and. ... Photodisintegration effectively reverses nucleosynthesis! Structure & Evolution of Stars 19. Structure & Evolution of Stars 20.

  7. Educational and Outreach talks and activities for Carolin Crawford ...

    https://people.ast.cam.ac.uk/~csc/newcv/2018talks.html
    24 Jul 2019: Nov. 20. Dark Energy. Students attending Villiers Park course. Nov. 20.

  8. Cambridge XMMSSC Internal pages

    https://people.ast.cam.ac.uk/~xmmssc/internal/
    10 Feb 2003: XMM Subaru Deep Survey (SDS) programme. Last modified: Mon Feb 10 20:16:49 2003.

  9. 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.

  10. Educational and Outreach talks for Carolin Crawford in 2009 ...

    https://people.ast.cam.ac.uk/~csc/newcv/2009talks.html
    24 Jul 2019: June. 20. The science and beauty of nebulae. Royal Astronomical Society public lecture. ... Mar. 20. The Planets. Talk to KS2 pupils at Dry Drayton primary school.

  11. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html
    26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation).

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