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41 - 50 of 363 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 363 match some words.

  1. Results that match 1 of 2 words

  2. Lecture 14 Introduction to Cosmology SDSS DR3, 7 2010AAT ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture14_slides.pdf
    20 Nov 2018: 2014). 100 150 200 2500. 0.2. 0.4. 0.6. 0.8. 1. r!

  3. PrimordialD_jun18.key

    https://people.ast.cam.ac.uk/~pettini/Primordial%20D%20Jun18
    5 Jul 2018: N(H I) = 2.5 1020 cm2. Fe/H = 1/200 solar. Very Metal Poor DLAs are the choice astrophysical environments for measuring the primordial abundance of deuterium.

  4. Estimate of the Number of CPU Nodes to Execute ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf
    29 Sep 2006: Data:. • Average of 200 Gb of science data per night (about 14 hours long). • ... Average night: 200 Gb/0.27 Gb = 740 images per night.

  5. Chapter 4 - Controls Reference

    https://people.ast.cam.ac.uk/~rgm/cirsi/pixcel/pixcel_19990428_help/chapter4.htm
    23 Jan 2000: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  6. Microsoft PowerPoint - wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_hst08.pdf
    7 Feb 2008: ACS image of 5Myr HD141569 shows dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.

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

    https://people.ast.cam.ac.uk/~csc/newcv/2014talks.html
    24 Jul 2019: Mar. 350, 200. Your place in the cosmos. Talk to high school pupils from Finland. ... Mar. 200. The Northern Lights. Talk at Public Open Evening, IoA.

  8. Chapter 2 : Operating the software

    https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter2.htm
    15 Nov 1998: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  9. Astronomy & Astrophysics manuscript no. letter_HD206893 c©ESO…

    https://people.ast.cam.ac.uk/~wyatt/mhcc16.pdf
    2 Dec 2016: Zuckerman & Song(2004) estimated an age of 200 Myr based on X ray, radial ve-locity and proper motion measurements. ... Us-ing an age of 200 Myr (respectively 800 Myr, 2 Gyr) and theAMES-Cond models (Baraffe et al.

  10. 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.

  11. Basic Debris Disk Model

    https://people.ast.cam.ac.uk/~wyatt/wyat06b.pdf
    21 Sep 2006: Dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.

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