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61 - 70 of 74 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 74 match some words.

  1. Results that match 1 of 2 words

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

    https://people.ast.cam.ac.uk/~wyatt/mmks15.pdf
    19 Jan 2015: 1 1 29/204 0.140.020.03 29/204 0.14. 0.020.03. 2 2 24/182 0.130.020.03 22/179 0.12. ... 6 1o 21/146 0.140.020.03 8/33 0.24. 0.060.09 7/49 0.14. 0.040.06 6/64 0.09.

  3. Draft version May 29, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf
    14 Sep 2015: Draft version May 29, 2015Preprint typeset using LATEX style emulateapj v. 5/2/11. A COMPACT CONCENTRATION OF LARGE GRAINS IN THE HD 142527 PROTOPLANETARY DUST TRAP. Simon Casassus1,2, Chris Wright3, Sebastian Marino1,2, Sarah T. Maddison4, Al

  4. Appendix XXX

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/appendix.doc
    16 Jun 2015: 23. M_ST4. DATA4. 53. AGND. GND5. 24. M_ST4. DATA4. 54. AGND. ... 22. RESET. 23. SAFETY GND. 24. NC. 25. NC. Changes. v1 Original form.

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

    https://people.ast.cam.ac.uk/~wyatt/pw15.pdf
    14 Sep 2015: Mon. Not. R. Astron. Soc. 000, 1–14 (2002) Printed 17 July 2015 (MN LaTEX style file v2.2). Double-ringed debris discs could be the work ofeccentric planets: explaining the strange morphology ofHD 107146. Tim D. Pearce? and Mark C. WyattInstitute

  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: CIRSI gives a whole time on one fill of liquid nitrogen in excess of 30 hours in downward looking mode and approximately 24 hours in upward looking mode.

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

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 Mar 2015: Theco-added spectrum consists of 27 observations of 20 minutesduration each, over 5 nights between 12 Nov 2013 and 24 Dec2013. ... albe. do. Qabs (24)Qsca (H)Qabs (H)Albedo. Figure 10. Scattering and absorption properties for silicate/organicgrains as a

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

    https://people.ast.cam.ac.uk/~wyatt/rw15.pdf
    17 Dec 2015: T =2. πb(2)3/2(α). (a2a1. )5/2  f 2(1 L2. L1. )24.

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

    https://people.ast.cam.ac.uk/~wyatt/kwbb14.pdf
    15 Jan 2015: arX. iv:1. 412. 0675. v1 [. astr. o-ph. EP. ] 1. Dec. 201. 4DRAF T VERS IONDECEMBER 3, 2014Preprint typeset using LATEX style emulateapj v. 5/2/11. EXO-ZODI MODELLING FOR THE LARGE BINOCULAR TELESCOPE INTERFEROMETER. GRANT M. K ENNEDY1, M ARK C.

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

    https://people.ast.cam.ac.uk/~wyatt/smw15.pdf
    15 Jan 2015: δE Gm (1 β)2ap. (1 2) , (24). and equating the two energies yields. ... 3. Allow-ing for capture into lower j resonances, the overall captureprobability into the 6:5 mean motion resonance for particleswith similar initial conditions is 0.24.

  11. proceedings2.dvi

    https://people.ast.cam.ac.uk/~optics/dazle/publications/5492-1022-dazle.pdf
    16 Jun 2015: 9.18 12351.9 68.99 48.9 12400.8 16.89 100 Some contamination. 9.24 12423.7 37.60 58.8 12482.5 7.88 100 Some contamination.

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