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  2. arX iv:a stro -ph/ 0603 608 v2 1 Se ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/dye.pdf
    28 Sep 2006: arX. iv:a. stro. -ph/. 0603. 608. v2. 1 Se. p 20. 06. Mon. Not. R. Astron. Soc. 000, 1–26 (2006) Printed 4 September 2006 (MN LATEX style file v2.2). The UKIRT Infrared Deep Sky Survey Early Data Release. S. Dye1, S. J. Warren2, N. C. Hambly3, N.
  3. NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE ...

    https://people.ast.cam.ac.uk/~wyatt/bbsg06.pdf
    28 Nov 2006: For exam-ple, the 70 m emission is well centered on the 24 m positions,typically within 100.
  4. aa2073.dvi

    https://people.ast.cam.ac.uk/~wyatt/wyat05b.pdf
    19 Apr 2006: For exam-ple, SCUBA observations at 850 µm have a limit of a few mJy(Wyatt et al.
  5. PDF/36/aa3391-05.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/wyat05c.pdf
    19 Apr 2006: The region of aligned orbits in this exam-ple corresponds to the parts of the orbits where the planetesi-mals are all somewhere between apocentre and pericentre (as.

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