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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. CIRSI-Technical Characteristics and Expected Astronomical Performance

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi_brief.html
    16 Jun 2015: 5.5' x 5.5'. 20.9' x 20.9'. 30.9. 0.42. INT. Prime f/3.3. ... NICMOS. MCT 256x256. 0.04-0.20. -. -. -. Notes:. (1) Survey Power is the product of the collecting area in m2 times the field of view in degrees, neglecting any losses due

  3. 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.

  4. 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

  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. 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".

  7. 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.

  8. 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.

  9. 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.

  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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