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31 - 40 of 109 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 109 match some words.

  1. Results that match 1 of 2 words

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

    https://people.ast.cam.ac.uk/~wyatt/pw15.pdf
    14 Sep 2015: Instead, we run simulations withaplt = 20, 30, 40 and 50 au (noting that the inner peak ofthe observed surface density profile is at 50 au, and thatthe planet’s initial semimajor ... Conversely, we find thatplanets with initial semimajor axes of 20 and

  3. /astro/p7scch2/AUMic/paper/figures/all.eps

    https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf
    16 Jun 2015: There is also an NW-SEasymmetry, with the NW side brighter than the SE side in-terior to 20 au. ... 37.5 – 42.5 r 00. 0.03 0.015 M1. 1.5 103 20 0.02.

  4. proceedings2.dvi

    https://people.ast.cam.ac.uk/~optics/dazle/publications/5492-1022-dazle.pdf
    16 Jun 2015: 9.99 13325.2 20.5 75.7 13401.0 3.81 80 Clean window. 2.2. Narrowband Filters.

  5. Appendix XXX

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc
    16 Jun 2015: SHUTTER_OPEN_DELAY:. % Delay for address to settle%. [ADDS_20 HOLD RES_I _RES_T H1 _CONVT UP CAMA WR_RM] CONTINUE;. ... ADDS_20 HOLD RES_I _RES_T H1 _CONVT UP CAMA WR_RM] CONTINUE;. % Save highest byte on the stack%.

  6. Draft version January 19, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf
    19 Jan 2015: 501. 0381. 3v1. [as. tro-. ph.E. P] 1. 5 Ja. n 20. ... that, for the planet-hosts, thebinary fraction is significantly lower than field stars forbinary semimajor axes <20 AU.

  7. https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt
    16 Jun 2015: GY-11 16:23:20.8 -24:17:21 2349.8-2601 16:23:49.8 -24:26:01 CRBR-14 16:23:17.3 -24:19:25 GY-10 ... 23:20.8 -24:17:08 2MASSW-J2049197-194432 20:49:19.74 -19:44:32.5 2MASSW-J2147446-264406 21:47:44.62 -26:44:06.6 2MASSW-J2206228-204705

  8. Project Reassessment Start Date

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc
    16 Jun 2015: It is more suited to a shallow survey to H(20 as indicated by Figure 2.2.1a. ... Short wavelength cut-on (micron) 0.85 0.85. Read noise (e- at 77K) < 20 < 5.

  9. MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/rw15.pdf
    17 Dec 2015: MNRAS 000, 1–14 (2015) Preprint 17 December 2015 Compiled using MNRAS LATEX style file v3.0. Dynamical Constraints on Outer Planets in Super-Earth Systems. Matthew J. Read1? and Mark C. Wyatt11Institute of Astronomy, University of Cambridge,

  10. https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000620.al

    https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000620.al
    16 Jun 2015: AM on 2000 Sep 24; standard zone = 0 hrs W For the night of: Tue, 2000 Jun 20 --- Wed, 2000 Jun 21 Local midnight = 2000 Jun 20, 23 hr UT, or

  11. Summary

    https://people.ast.cam.ac.uk/~optics/cirpass/summary.bak
    16 Jun 2015: Last modified: Wed Nov 24 12:12:20 1999.

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