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  1. Results that match 1 of 2 words

  2. 19 Apr 2006: "!# $&% ' )(# -,/.0-%12 &!$3542,67,98/:<;=?> @A>BDCFEGIHJ8K>L>MONPEQRCFSUTV8WX>YZ>L[GIEE]E[_7=?>Ya>bCFcXdGIHe_UNPEgfMhC[cA:QUeiPGkjEmlPG#QU_UmSn;opQqGI_U_#8rMhC[cX:Qq]iPG$st8vuFwPwPx>yopzV>|{-}8vuP{}Ic>yopQU]#GpPwgfT2C[Qqi:NPdEiV9bKhw{Pu&}&}P<As>.
  3. 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.
  4. 19 Apr 2006: "! $#&%(')! ,.-/%103246587797: 0<;=>&?%/3#60A@ B4%)CD0CEGFHI6KJ&0ML80ONPRQ8%S 4T0. UWVYXOZ [MV6]AXV_ba c&dfehgjiZ k.l<]m.XOV$c=nPo$Zpp.V6qUhal VC]rsZ qoftuvxw=y"z. {}|x|C) 9(A6Wf69O6AR.E&RAAA9E9 //.¡¢E£¤E(¥ª«¢¥ª<E4OP/GK=. |Y|&µEºA)»|&{f|
  5. arX iv:a stro -ph/ 0601 592 v1 26 J ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/hewettetal.pdf
    28 Sep 2006: The low sensitivityof most optical CCD detectors at 1 µm, coupled with therelatively bright sky-background curtailed interest from op-tical astronomers.
  6. ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf
    19 Apr 2006: ApJ accepted, 7 November 2005Preprint typeset using LATEX style emulateapj v. 04/21/05. DUST IN RESONANT EXTRASOLAR KUIPER BELTS — GRAIN SIZE AND WAVELENGTH DEPENDENCEOF DISK STRUCTURE. M. C. Wyatt1. UK Astronomy Technology Centre, Royal
  7. SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...

    https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf
    19 Apr 2006: 4.2. Modelingg the SED. The spectral energy distribution (SED) of Corvi from op-tical to submillimeter wavelengths is plotted in Figure 4.
  8. 28 Sep 2006: tuwv »¿ x v , v &,-3'T$É!' v $%3& v x2#AÎG&ÖP-!1Y, uwv x v |, v &,-3'i3&(,) yGv 3' v )s%.;.
  9. 19 Apr 2006: " $#%&%&' ()" #$%%'-,.0/(12&34657798:";" =<>? @$$A$>;"? BC? ";D= ;" EF46 "9/ GHJI"K"KMLBNPOQ R9SOETUQ VFW"OXTMY!Z[QS W"OXW"]BV. GTMY_OXVFW"O. (a Nb?K"K&c K"K"K"KdUe(K"K"K"K"K"K"K"K"K"K"K"K"K"K"KMe. fhgji kmlon_pqnsr turwv xzy|{|}ns{|r {|wi}_. 6sJ
  10. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: To probe the nature of the Vega disk further, wehave fitted it with models including realistic grain op-tical properties.
  11. arX iv:a stro -ph/ 0311 593 v1 26 N ...

    https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf
    19 Apr 2006: 10 µm) to spiral inwards toward the star.Which of these two effects is dominant depends on the op-tical depth of the dust disk, but for all but the most

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