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21 - 30 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. HAWAII SAM MICROCODE

    https://people.ast.cam.ac.uk/~optics/cirsi/SAM/cirsi_sam_microcode_22dec97.html
    16 Jun 2015: 1714 1500 2.20. 2000 and above 1714 2.35. (note intermediate rates all work.

  3. https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000519.al

    https://people.ast.cam.ac.uk/~optics/cirsi/ing/2000a/20000519.al
    16 Jun 2015: AM on 2000 Sep 24; standard zone = 0 hrs W For the night of: Fri, 2000 May 19 --- Sat, 2000 May 20 Local midnight = 2000 May 19, 23 hr UT, or ... evening twilight: 12 08 Morning twilight: 5 48 GDT; LMST at morning twilight: 19 29 12-degr twilight: 21 55

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

    https://people.ast.cam.ac.uk/~wyatt/smw15.pdf
    15 Jan 2015: of 2π 102, and semimajoraxis chosen randomly and uniformly between 2.20 ap and. ... 105. 2x105. 3x105. 4x105. 5x105. 6x105. 7x105. 0 20 40 60 80 100.

  5. /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.

  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. arX iv:1 501. 0318 1v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/asgw15.pdf
    15 Jan 2015: n 20. 15. Astrophysical Journal, in press. The Inner Disk Structure, Disk-Planet Interactions, and. ... 0.0. 0.1. 0.20.3. Dis. tanc. e [". ]. Gaussian Centers Above Midplane.

  8. arX iv:1 412. 0675 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwbb14.pdf
    15 Jan 2015: 0. 20. 40. 60. 80. Incl. inat. ion. (deg. ). 0.30.

  9. CIRSI: the Cambridge Infrared Survey Instrument for Wide-Field…

    https://people.ast.cam.ac.uk/~optics/papers/CIRSI_SPIE_4008_146.doc
    16 Jun 2015: This makes it ideally suited to large area programs with limiting magnitudes of H=19-20. ... Here the delivered pixel at the f/7.5 cassegrian focus is 0.20".

  10. 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,

  11. 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%.

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