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101 - 109 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. arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf
    25 Nov 2015: 20 0 20 Offset("). 20. 0. 20. Offs. et(". ). 20 0 20 Offset("). ... 20 0 20 Offset("). 20 0 20 Offset("). X. 20 0 20 Offset(").

  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: 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".

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

    https://people.ast.cam.ac.uk/~wyatt/kmmg15.pdf
    10 Mar 2015: The disc is well re-solved so we use a 20′′ radius aperture that is centred on the. ... Afteraperture correction we find a flux density of190 6 mJy at 70µm, and of141 20 mJy at 160µm.

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

    https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf
    14 Sep 2015: 2013) (here we use Rs = 148 AU, and anazimuthal contrast in surface density of c = 20.0). ... Thescale-height H is given by. H(r) = 20.0( r. 130 AU.

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

    https://people.ast.cam.ac.uk/~wyatt/blrf15.pdf
    14 Sep 2015: The panel sec-ond from the bottom ‘(c)’) shows no low-frequency (10 – 20 day). ... The deep-est τ = 20% dimming event at D1500 thus implies that at least.

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

    https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf
    2 Nov 2015: 0.90. 1.00. 1.10. 1.20. EPIC 203895983. 2060 2076 2092 2108 2124 2140. ... Integrationtimes of a few minutes yielded SNR 20–90 in the Li I6708 Å line (Table 2).

  8. https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_atmosph_transm…

    https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_atmosph_transmission_nir.txt
    16 Jun 2015: # # rgm copied from #http://www.jach.hawaii.edu/JACpublic/UKIRT/astronomy/calib/atmosph_short.lines # 0.9000 9.60168E-01 0.9005 9.60579E-01 0.9010 9.61084E-01 0.9015 9.61924E-01 0.9020 9.63728E-01 0.9025 9.67188E-01 0.9030 9.72331E-01 0.9035 9.78154E

  9. 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.

  10. 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.

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