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61 - 70 of 77 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 77 match some words.

  1. Results that match 1 of 2 words

  2. 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.

  3. 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.

  4. Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...

    https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf
    2 Nov 2015: EPIC 203410665 (V V896 Sco) and 203937317(DoAr 24) are both well-known members of ρ Oph thathave been studied in the near-IR (e.g., Furlan et al. ... 204630363 407050 K7.5 0.810.130.13 24.2118.2 — — — 15 C F/(P)TD.

  5. 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.

  6. Next Generation Very Large Array Memo No. 6Science Working ...

    https://people.ast.cam.ac.uk/~wyatt/ihmg15.pdf
    24 Oct 2015: 24. 5 Chemical evolution of the star and planet forming environ-ment 275.1 Complex organic molecules in Hot Molecular Cores. ... The cyan contours are –6, –3, 3, 6, 12, 24, 48, 96, 192 σI, whereσI = 19.5µJy bm1 is the rms noise in the Stokes I map.

  7. arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf
    25 Nov 2015: 110411† 154 7.0‡ 67.3 7.0‡. 125162 272 15‡ 142 12‡. 183324† 25.4 1.1 17.2 3.3198160 30.7 1.2 14.3 1.7221756† ... Star (HD) µra(mas/yr) µdec(mas/yr) vrad(km/s) Parallax(′′ ) Distance (pc). 11413 -48.27 0.24 -4.42 0.30 3.0 0.7 12.96

  8. 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.

  9. Project Reassessment Start Date

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc
    16 Jun 2015: 5.5.2 SAM Code GOTOBUTTON _Toc361307169 PAGEREF _Toc361307169 24. 5.5.3 Transputer GOTOBUTTON _Toc361307170 PAGEREF _Toc361307170 24. ... 5.5.4 Data Output Format GOTOBUTTON _Toc361307171 PAGEREF _Toc361307171 24. 5.6 Computer Interface GOTOBUTTON

  10. 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

  11. 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

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