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  2. Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: For the clustering of data and to guide the interpretation, wealso extracted environmental data from either the adaptive op-tics telemetry3 or the Astronomical Site Monitor (ASM) of theCerro Paranal Observatory4. ... We found much lower correlation rates
  3. arX iv:1 709. 0841 4v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/mcka17.pdf
    26 Sep 2017: three disks. For HD 131488, even the 13CO line is op-. ... tically thick with an optical depth of 5.7, while for. HD 121191 and HD 121617 this line was found to be op-tically thin.
  4. ms.dvi

    https://people.ast.cam.ac.uk/~wyatt/wmke16.pdf
    10 Nov 2016: With the advent of an extreme adaptive op-tics instrument like the Spectro-Polarimetric High-contrastExoplanet REsearch (SPHERE; Beuzit et al.
  5. 23 Dec 2016: It summarizes previous findings aswell as results from this work. EC acknowledges support from NASA through HubbleFellowship grant HST-HF2-51355 awarded by STScI, op-erated by AURA, Inc.
  6. 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|
  7. arX iv:1 702. 0512 3v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/bfwv17.pdf
    5 May 2017: The calculations sofar have focused on the geometrical optical depth of the op-tically thin dust, τ. ... edge. Such dust, how-ever, would produce a detectable infrared excess, as for op-tically thin discs, there is insufficient gas released for
  8. 17 Jan 2019: We can estimate a minimum CO mass by assuming that the CO emission is marginally op-.
  9. 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
  10. arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf
    27 Jan 2016: 2014; Veillet et al. 2014). The LBT is locatedon Mount Graham in southeastern Arizona and is op-erated by an international collaboration among institu-tions in the United States, Italy, and ... The op-tics provide a field of view of 1010 arcsec2 with
  11. arX iv:1 201. 1911 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf
    12 Jan 2012: 2004), an adaptive op-tics image taken using the Lick Observatory Shane 3m tele-scope with the IRCAL near-IR camera as an ongoing search forfaint companions of stars in the ... To try and resolve this issue we obtained an adaptive op-tics image of 99 Her

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