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21 - 30 of 31 search results for katalk:za33 24 |u:people.ast.cam.ac.uk where 0 match all words and 31 match some words.

  1. Results that match 1 of 2 words

  2. MNRAS 000, 1–11 (2018) Preprint 27 June 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/sbbc18.pdf
    31 Jul 2018: MNRAS 000, 1–11 (2018) Preprint 27 June 2018 Compiled using MNRAS LATEX style file v3.0. The KIC 8462852 Light Curve From 2015.75 to 2018.18Shows a Variable Secular Decline. Bradley E. Schaefer1?, Rory O. Bentley1, Tabetha S. Boyajian1, Phillip H.

  3. Mon. Not. R. Astron. Soc. 000, 1–23 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kmwk18.pdf
    22 Nov 2018: 8715. 16. 80 88 96 104. R0. 0.06. 0.12. 0.18. 0.24. ... 0.06. 0.12. 0.18. 0.24. h. h = 0. 160. 060. 09.

  4. M. Pettini: Introduction to Cosmology — Lecture 10 FLUCTUATIONS ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture10.pdf
    6 Nov 2018: IRJνIRJν. = 2y (10.23). and. y =. kT. mec2σT ne dl (10.24). ... Note that the so-called. Compton y parameter in eq. 10.24 increases with T, since the temperaturedetermines the average energy transfer per scattering event.

  5. Draft version April 5, 2018Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mmkw18.pdf
    5 Apr 2018: R1L,α and fR, and a likelihood function described. by Eq. 24 in Kelly (2007), assuming Gaussian errors on. ... Su et al. 2006) at 24 µm (taken. as the largest between 0.3mJy and 2% of the star’s 24.

  6. M. Pettini: Introduction to Cosmology — Lecture 16 DARK ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture16.pdf
    22 Nov 2018: 16.22 is: 〈. v2〉. = 3 (880 km s1. )2(16.24). The half-mass radius is trickier. ... Experimentsusing solar, atmospheric, and reactor neutrinos have measured mass dif-. 24.

  7. Draft version January 1, 2018Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mwoa18.pdf
    2 Jan 2018: Draft version January 1, 2018Typeset using LATEX twocolumn style in AASTeX61. MOLECULAR RECONNAISSANCE OF THE β PICTORIS GAS DISK WITH THE SMA:. A LOW HCN/(COCO2) OUTGASSING RATIO AND PREDICTIONS FOR FUTURE SURVEYS. L. Matrà,1, D. J. Wilner,1 K.

  8. MNRAS 000, 1–21 (2017) Preprint 14 June 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/wvkb17.pdf
    14 Jun 2018: MNRAS 000, 1–21 (2017) Preprint 14 June 2018 Compiled using MNRAS LATEX style file v3.0. Modelling the KIC8462852 light curves: compatibility of the dipsand secular dimming with an exocomet interpretation. M. C. Wyatt1?, R. van Lieshout1, G. M.

  9. arX iv:1 801. 0542 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmp18.pdf
    18 Jan 2018: The best fit power-law index for this model (χ2 = 5.1)is p = 24 2, which corresponds to a FWHM of only 5au.

  10. MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mcwb18.pdf
    31 Jul 2018: Band 6 - 12m 24, 27-30 Apr 2017 236.4 6.8 0.′′67 0.′′66 (2.9) 41 and 312 J12290203 J12290203 J12151654Band 7 - 12m 11 Dec 2016 48.8

  11. MNRAS 479, 2649–2672 (2018) doi:10.1093/mnras/sty1677Advance Access…

    https://people.ast.cam.ac.uk/~wyatt/kwtm18.pdf
    30 Jul 2018: 2 1) (33, 29, 24, 21,. 18, 16, 14 km s1, for planet b to h) for parallel orbits at impactand would be maximal for radial encounters at.

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