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  1. Results that match 1 of 2 words

  2. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 Apr 2006: This 200-AU-sized regioncoincides with the slightly tilted inner disk identified optically withthe Hubble Space Telescope5. ... The possible relationship of these components has yetto be explored, but the lower inferred temperatures of the clumpparticles
  3. 58419 1321..1340

    https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf
    19 Apr 2006: RESONANT TRAPPING OF PLANETESIMALS BY PLANET MIGRATION: DEBRIS DISK CLUMPSAND VEGA’S SIMILARITY TO THE SOLAR SYSTEM. M. C. WyattUK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, UK; wyatt@roe.ac.uk. Received 2003 June 11;
  4. aa2073.dvi

    https://people.ast.cam.ac.uk/~wyatt/wyat05b.pdf
    19 Apr 2006: 1984). This excess emission comes from dust in orbitaround the stars and its relatively cold temperature implies thatit resides at large distances from the stars, 30–200 AU, some-thing which ... 2003a) and IRAS observations at 60 and 100 µmhad 3σ
  5. ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf
    19 Apr 2006: ac-count and 200 dust particles were produced with exactlythe same positions and velocities as the parent popula-tion. ... for the librationparameters to be fitted for each particle, and the meanparameters for each population of 200 dust grains to
  6. arX iv:a stro -ph/ 0311 593 v1 26 N ...

    https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf
    19 Apr 2006: HD207129 G0V 15.6 1.0 104 Spline 603022901660 8. HD22049 ǫ Eri K2V 3.22 1.1 104 Best fit model 730 200 10HD39060 β Pic A5V 19.3 3 ... HD109085 0.0 4.2 4.0 180 40HD38393 0.0 2.7 0.4 200 50HD48682 0.0 2.3 7.0 71 15a.
  7. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: higher surface brightness at r >200 AU compared to the r4 power law. ... but has slightlyhigher surface brightness at r > 200 AU compared to ther4 power law.
  8. Basic Debris Disk Model

    https://people.ast.cam.ac.uk/~wyatt/wyat06b.pdf
    21 Sep 2006: Dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.
  9. Data Flow System Document Title: VISTA Data Reduction Library ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010.pdf
    28 Sep 2006: Data Flow System Document Title: VISTA Data Reduction Library Design Document Number: VIS-SPE-IOA-20000-0010 Issue: 1.5 Date: 2006-09-28 Document Prepared by:. Jim Lewis Peter Bunclark Simon Hodgkin (CASU). Signature and Date:. Document Approved by:.
  10. Document Title: VISTA Infra Red Camera Calibration Plan Document ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0002.pdf
    28 Sep 2006: event that observations of a secondary photometric standard field with a density of 100-200 objects per detector are available, then the illumination correction can be measured by looking at the
  11. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v3p0.pdf
    6 Jun 2006: Execute tiles that overlap with 200 deepest XMM pointings. • Fornax galaxy cluster(50deg2). ... The black filled circles are 200 deep public XMM pointings from the 2XMMcatalogue.

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