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  2. 8 Mar 2021: 2017).Recently, this trend has been supported by new obser-vations from the Hunt for Observable Signatures of Ter-restrial planetary Systems (HOSTS, Danchi et al. ... This new modelconsiders not only the spatial density profile as in themodels of Wyatt
  3. Draft version February 20, 2021Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/wgml21.pdf
    19 Jul 2021: for infrared excesses. 5. SUMMARY AND CONCLUSIONS. We have presented a new catalog of Spitzer 3.6 micron (IRAC1) and 4.5 micron (IRAC2) infrared photometry of.
  4. MNRAS 000, 1–15 (2020) Preprint 29April 2021 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/ckkm21.pdf
    29 Apr 2021: It is one of very fewnearbyM-dwarfs knownto host a debris disc and of these has by far the lowest stellarmass.We present new resolvedobservationsof thedebris disc aroundFomalhautCwith theAtacamaLargeMillimetreArraywhich allow us ... This paper considers
  5. Publications of the Astronomical Society of Australia (PASA)doi:…

    https://people.ast.cam.ac.uk/~wyatt/khna21.pdf
    23 Nov 2021: below 2000 K) than probed by opticalforbidden lines. SMI, with its high spectral resolutionand sensitivity, will break new ground in the study ofgas dispersal in protoplanetary disks. ... The C/O ratio also has an impact on secondaryatmospheres, as these
  6. MNRAS 000, 1–23 (2020) Preprint 14 June 2021 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/lmwk21.pdf
    16 Jul 2021: In this work we present new high-resolution (sub-arcsec)ALMA observations of q1 Eri to characterise its asymmetric outerbelt and to consider the relationship of that belt to the planetarysystem

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