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  2. Erin E Hayes

    https://people.ast.cam.ac.uk/~eeh55/resume.html
    2 May 2024: The researchers give a presentation about their science and then help the students create art which visualizes the data from the presentation in a new way.
  3. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: Therefore, tackling a prime objective of exoplanet science and understanding how unique or common planets like our Earth are in our galactic neighborhood will require a new, dedicated approach. ... below). 15. 2.3 Timing for a space-based mid-infrared
  4. Astronomy & Astrophysics manuscript no. aa ©ESO 2024April 9, ...

    https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf
    9 Apr 2024: The new ALMA observa-tion is marked as a black circle, and the blue circle represents the fluxat the stellar position. ... Con-sequently, the broad structure of the Herschel observations seessmaller grains whose distribution is modified by radiation
  5. 22 Mar 2024: Science (New York, N.Y.) 233,869–72 (1986). [21] Maurette, M., Brack, A., Kurat, G., Perreau, M. &
  6. MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/hwd22.pdf
    22 Mar 2024: We describethe new mid-IR observations of Beta Pic in Section 2 and the datareduction procedures in Section 3. ... 5 DISCUSSION. In the following sections, we discuss new constraints that can beobtained in light of the newobservations under theories
  7. MNRAS 000, 1–17 (2033) Preprint 19 June 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf
    22 Mar 2024: In order to do so, we de-velop a new extension of Frankenstein (Jennings et al. ... The new version of frank includes now an option to consider opticallythin or thick emission.
  8. Draft version July 18, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 Mar 2024: any detections of circumstellar dust emission. These data provide new limits on dust belt fractional luminosities and. ... 2007a). Najita et al. (2022) used new coagulation models to assess the possibility that the observed population of cold debris.
  9. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: An ALMA Survey of M-dwarfs in the Beta Pictoris Moving Group withTwo New Debris Disc Detections. ... 2018),further solidifying the BPMG as a good candidate sample to searchfor new discs.
  10. Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: Large surveys provided new insights about the frequency and properties of massive sub-stellar companions withseparations from 5 to 300 au.Aims. ... A new planetary characterisation algorithm, based on the RSM framework, is developed and testedsuccessfully
  11. MNRAS 000, 1–17 (2022) Preprint 28 June 2022 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf
    22 Mar 2024: In 2 we present and describe a new model thattakes into account photodissociation, vertical diffusion, ionisation,and viscous evolution of gas continuously released in a planetesi-mal belt.

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