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11 - 20 of 57 search results for watson |u:people.ast.cam.ac.uk

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  2. ApJ409619o.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwcm11.pdf
    23 Feb 2012: was performed, with 1 cycle of 6 s integration at eachposition (Watson et al.

  3. arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf
    7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot,

  4. arX iv:1 310. 6936 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/gkte13.pdf
    28 Oct 2013: von Braun K. et al., 2011, ApJ 729, L26. Watson C.A.

  5. https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt
    16 Jun 2015: Spot a 00:47:33.410 -25:17:13.6 Spot i 00:47:33.013 -25:17:18.12 Spot n 00:47:33.063 -25:17:17.20

  6. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf
    5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

  7. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090923.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090923.txt
    28 Sep 2009: MJI is in communication with Watson Varricatt regarding the low light level non-linearity tests and also a revisit of the normal non-linearity tests. ... Watson and MJI will also be comparing dome flats with twilight sky flats.

  8. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p1.pdf
    5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

  9. Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf
    5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.

  10. MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/kw20.pdf
    18 Aug 2020: MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled using MNRAS LATEX style file v3.0. Solution to the debris disc mass problem:planetesimals are born small? Alexander V. Krivov1? and Mark C. Wyatt21Astrophysikalisches Institut und

  11. Space Science Reviews manuscript No.(will be inserted by the ...

    https://people.ast.cam.ac.uk/~wyatt/wj16.pdf
    15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant

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