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11 - 20 of 32 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 32 match some words.

  1. Results that match 1 of 2 words

  2. New Page 1

    https://people.ast.cam.ac.uk/~optics/people/cdm_CV_130509.htm
    16 Jun 2015: This involved using the One-Mile Radio Telescope of the Mullard Radio Astronomy Observatory to observe a sample of 200 bright radio sources in the 3C revised catalogue, at galactic latitudes

  3. MGB thesis Chapter 2

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter2.htm
    16 Jun 2015: 1.05. 150 - 300. Indium Gallium Arsenide (InGaAs). 0.7. 1.7. 77 - 200.

  4. https://people.ast.cam.ac.uk/~optics/dazle/sky-data/ukirt_sky_ramsey_e…

    https://people.ast.cam.ac.uk/~optics/dazle/sky-data/ukirt_sky_ramsey_etal.dat
    16 Jun 2015: 196 1.29700 3408.63 197 1.29850 3794.42 198 1.29990 4543.59 199 1.30140 4584.77 200 1.30280 4085.07 201 1.30420 3724.87 202 ... 75750 202.051 199 1.75880 511.795 200 1.76010 1403.21 201 1.76140 4458.84 202 1.76270 12575.5 203 1.76400 13281.0 204 1.76530

  5. Chapter 2 - Operating the software

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter2.htm
    16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  6. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/blrf15.pdf
    14 Sep 2015: There are modulations in the raw flux data at the 200 ppmlevel which are visible by eye. ... 5. Time (BJD-2454833). No. rma. lize. d f. lux. 190 200 210 220 230 240.

  7. https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduct…

    https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduction_manual
    16 Jun 2015: It is approximately the size of one chip, i.e., 200 arcsec on a side.

  8. MGB thesis Chapter 3

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm
    16 Jun 2015: [Chapter 3: Camera. Outline. This chapter describes the near infrared camera built for COAST. It examines the properties required from the camera system, the range of devices available and the factors involved in the choice of detector. The design,

  9. Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pw15.pdf
    14 Sep 2015: A /. yr-1. 108. 106. 104. 102. 100. a / au0 50 100 150 200. ... 0.2. 0.4. 0.6. 0.8. r / au0 50 100 150 200.

  10. MGB thesis Chapter 4

    https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter4.htm
    16 Jun 2015: The exposure times were 50, 100 and 200 milli-seconds. Results. Signal (e. -.

  11. arX iv:1 503. 0207 3v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 Mar 2015: for material uniformlydistributed around a circular narrow ring at 200 au, with thein-clination derived from the 70µm PACS image. ... models the inner edge is around 30 au, and theouter edge around 200 au.

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