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  1. Results that match 2 of 3 words

  2. MNRAS 000, 1–11 (2015) Preprint 9 November 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/khhw18.pdf
    9 Nov 2018: The solution to remove this class of events is to empiri-cally look at the comet entry and exit parameters, θ and λ.If one was found to be more than ... MNRAS 000, 1–11 (2015). 10 GMK et al. requirement less stringent.
  3. M. Pettini: Introduction to Cosmology — Lecture 16 DARK ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture16.pdf
    22 Nov 2018: Neutrinos 0.001. Photons (CMB) 5 105. Comparing the entries in the third and fourth row, we see that stars andtheir remnants (mostly white dwarfs) account for less than 10% of ... In any case, the search continues for a WIMP that may fit theastronomical
  4. 18 Apr 2022: Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED ESO 2022April 11, 2022. Large Interferometer For Exoplanets (LIFE):. I. Improved exoplanet detection yield estimates for a large mid-infraredspace-interferometer mission. S.P. Quanz1,
  5. Analysis of the Herschel DEBRIS Sun-like star sample

    https://people.ast.cam.ac.uk/~wyatt/skwl18.pdf
    19 Feb 2018: The requirement for planetesimals,themselves a step in the planet formation process, makes debrisdiscs a fundamental component of planetary systems. ... 2013), who use a 3σ excess detection at any PACS wavelengthas their disc detection requirement.
  6. MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/lwkk22.pdf
    29 Sep 2022: MNRAS 000, 1–21 (2022) Preprint 28September 2022 Compiled usingMNRASLATEXstyle file v3.0. High resolution ALMA and HST imaging of 𝜅 CrB: a broad debrisdisc around a post-main sequence star with low-mass companions. J. B. Lovell1,M.C.Wyatt1,
  7. Mon. Not. R. Astron. Soc. 000, 1–22 (2013) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/jwbv14.pdf
    11 Mar 2014: In mathematical termswe may write this requirement as. v. vk |v(t t) v(t)|. ... This arisesfrom the requirement that the new orbit of a particle must passthrough the point at which the kick is applied that is responsiblefor the apocentre and pericentre
  8. arX iv:1 402. 1184 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/dawk14.pdf
    10 Feb 2014: arX. iv:1. 402. 1184. v1 [. astr. o-ph. SR. ] 5. Feb. 201. 4. Spatially resolved imaging of the two-component η Crv debris disk with Herschel. G. Duchêne1, P. Arriaga. Astronomy Department, University of California, Berkeley, CA 94720, USA. and.
  9. arX iv:0 911. 3426 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/pgdm09.pdf
    19 Nov 2009: Volume limitedsamples satisfy these requirements, and as well as maximis-ing the proximity of the targets, the stars nearest the Sunare very widely studied. ... Where compo-nents are not resolved in any catalogues we have used, wejust give a single entry
  10. Data Flow System Document Title: VISTA Data Reduction Library ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010_latest.pdf
    7 Jun 2007: DRS dictionaries Update vircam_standard_process, modify vircam_jitter_microstep_process, and modify entries in table 10-1. ... 0001, issue 3.2 2005-02-24. [RD 3] VISTA Science Requirements Document, VIS-SPE-VSC-00000-0001, issue.

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