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MNRAS 000, 1–11 (2018) Preprint 27 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/sbbc18.pdf31 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. -
Mon. Not. R. Astron. Soc. 000, 1–23 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kmwk18.pdf22 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. -
M. Pettini: Introduction to Cosmology — Lecture 10 FLUCTUATIONS ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture10.pdf6 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. -
Draft version April 5, 2018Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mmkw18.pdf5 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. -
M. Pettini: Introduction to Cosmology — Lecture 16 DARK ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture16.pdf22 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. -
Draft version January 1, 2018Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mwoa18.pdf2 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. -
MNRAS 000, 1–21 (2017) Preprint 14 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/wvkb17.pdf14 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. -
arX iv:1 801. 0542 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/kmmp18.pdf18 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. -
MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mcwb18.pdf31 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 -
MNRAS 479, 2649–2672 (2018) doi:10.1093/mnras/sty1677Advance Access…
https://people.ast.cam.ac.uk/~wyatt/kwtm18.pdf30 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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