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1 - 10 of 19 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 19 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. 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.

  5. 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.

  6. 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.

  7. 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.

  8. 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.

  9. 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

  10. 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.

  11. Microsoft PowerPoint - wyattpub

    https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf
    24 Apr 2007: Spiral structure at 200 AU implies planet at 150 AU• Same structure seen in Saturn’s rings (Charnoz et al. ... Numerical integrations of star, migrating planet, 200 planetesimalsgiving capture probabilities for 3:2 resonance:.

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