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1 - 10 of 20 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 20 match some words.

  1. Results that match 1 of 2 words

  2. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html
    3 Sep 2007: artdata. A full-well capacity of 200,000 electrons was used for the saturation level.

  3. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 Jun 2007: Dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.

  4. Data Curation at CASU

    https://people.ast.cam.ac.uk/~wfcam/talks/vdfs_jrl.ppt
    9 Feb 2007: 200-500 Gb/night expected for VISTA public surveys. Rice tile compression can save factors of 3-4 in 32 bit integer data.

  5. arX iv:0 704. 0873 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf
    18 Apr 2007: 200. 7. Mon. Not. R. Astron. Soc. 000, 1–6 (2006) Printed 9 April 2007 (MN LATEX style file v2.2). ... Doppler systems arepredicted here to form from 5-200 Jupiter masses of gas inthe disk, enough to make gas giant planets.

  6. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061207.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061207.txt
    31 Jan 2007: These 200 tapes probably only amount to about 1 Gbyte of data but are currently being ingested.

  7. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/
    3 Sep 2007: artdata. A full-well capacity of 200,000 electrons was used for the saturation level.

  8. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.pdf
    5 Jun 2007: a factor of 200:1 based onthe well established space densities of the foreground L and T dwarfs. ... Observing efficiency % per tile - - 73.3 - 69.9Time for 8,200 sq deg = 5467 tiles of 1.5 sq degTotal Elapsed Hours - - 373 - 391.

  9. 842 Publications of the Astronomical Society of the Pacific, ...

    https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf
    18 Sep 2007: typesystems) and young Sun-like stars (20 among 200 of the Gand K stars). ... Forinstance, with 200 stars per sample, a 15% difference in de-tection rate can be identified at the 3j level.

  10. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf
    5 Jun 2007: The Y-J colour is ESSENTIAL since the so called ’rare’ L and T dwarfs outnumberthe quasars by a factor of 200:1 based on the well established space densities of ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467

  11. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p1.pdf
    5 Jun 2007: a factor of 200:1 based onthe well established space densities of the foreground L and T dwarfs. ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467 tiles of 1.5 sq degTotal Elapsed Hours - - 373 - 391.

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