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1 - 10 of 65 search results for KaKaoTalk:po03 op |u:people.ast.cam.ac.uk where 0 match all words and 65 match some words.

  1. Results that match 1 of 2 words

  2. ����������� ��� ������������ ������� �!�"���…

    https://people.ast.cam.ac.uk/~wyatt/wyat05a.pdf
    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

  3. ��������� ��� �������� �� ������������� ��� "!# $�&% '�…

    https://people.ast.cam.ac.uk/~wyatt/wyat03a.pdf
    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>.

  4. ��������� �� ���������������������������������!…

    https://people.ast.cam.ac.uk/~wfcam/ukreview/wfcam_instrument.pdf
    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%.;.

  5. ��������� �� ��������������������� �������� ����������� "!…

    https://people.ast.cam.ac.uk/~wyatt/wdt00.pdf
    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|

  6. 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.

  7. Publications of the Astronomical Society of Australia (PASA)doi:…

    https://people.ast.cam.ac.uk/~wyatt/khna21.pdf
    23 Nov 2021: The HD J = 2 1 line is stronger for low mass op-tically thin disks (1019 W m2) and fainter for opticallythick massive disks (1018 W m2).Since the line fluxes ... Due to the lower op-tical depth with respect to the main isotopologue, the13CO transitions

  8. Planetary System DynamicsPart III Mathematics / Part III Astrophysics …

    https://people.ast.cam.ac.uk/~wyatt/psd_eg1.pdf
    29 Sep 2023: e) Derive an expression for the distance of the particle P from the geometric centre of the ellipse O, andhence show that to first order in eccentricity the distance OP is

  9. Observing guide for CIRSI (WFIRC) at LCO du Pont ...

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html
    16 Jun 2015: 2 FILTER7=Hn FILTER6=Jn FILTER5=Hl FILTER4=Hx FILTER3=Hs FILTER2=Jg FILTER1=Op FILTER0=Dk 13) Contact info, phone numbers, etc LCO during day this number is routed to

  10. Observing guide for CIRSI (WFIRC) at LCO du Pont ...

    https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html
    16 Jun 2015: 2 FILTER7=Hn FILTER6=Jn FILTER5=Hl FILTER4=Hx FILTER3=Hs FILTER2=Jg FILTER1=Op FILTER0=Dk 13) Contact info, phone numbers, etc LCO during day this number is routed to

  11. Noname manuscript No.(will be inserted by the editor) Space-based ...

    https://people.ast.cam.ac.uk/~wyatt/dlab18.pdf
    31 Jul 2018: JPL Publication. Lawson PR, Lay OP, Johnston KJ, Beichman CA (2007) Terrestrial PlanetFinder Interferometer Science Working Group Report. ... NASA STI/ReconTechnical Report N 8. Lay OP (2004) Systematic Errors in Nulling Interferometers.

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