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  2. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: 2018) and 24% of A-typestars (Thureau et al. 2014), but only detected two excesses aroundM-types (GJ 581; Fomalhaut C; Lestrade et al. ... 46 15.0 - 313.7 7.0 31.05.18 0.8 J0141-0928, J0006-0623BD30 397 B 30.47 44 15.1 - 500.2 5.6 24.08.18
  3. Cambridge Enterprise Venture Partners – Cambridge Enterprise

    https://www.enterprise.cam.ac.uk/for-external-organisations/opportunities-to-invest/cambridge-enterprise-venture-partners/
    27 Mar 2024: Join CEVP - a membership-only forum for investors who have an interest in early opportunities originating from the University of Cambridge.
  4. ccdc.cavity — CSD Python API 3.1.0 documentation

    https://downloads.ccdc.cam.ac.uk/documentation/API/_modules/ccdc/cavity.html
    28 Mar 2024: 16, TRP=17, TYR=18, VAL=19, UNK=20, ASX=21, GLX=22, NAD=23, NAP=24, FMN=25, MTX=26, HEM=27, ATP=28, COA=29, C=30, A=31,
  5. Joint CEENRG / CCI Conservation Seminar - Dr Ivan Hajdukovic |…

    https://www.conservation.cam.ac.uk/events/joint-ceenrg-cci-conservation-seminar-dr-ivan-hajdukovic
    26 Mar 2024: Date:. Wednesday, 24 April, 2024 - 12:00 to 13:00. Event location:.
  6. MNRAS 000, 1–17 (2022) Preprint 28 June 2022 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf
    22 Mar 2024: 𝑡vis =. 𝜋𝑟Δ𝑟. 3︁2ln(2)𝜈. 𝑟Δ𝑟2𝜈. (24). With this definition, the steady-state surface density ( ¤𝑀+/(3𝜋𝜈)) isindependentofΔ𝑟,andmatchesthesurfacedensityobtainedsolvingthe radial viscous evolution and the
  7. 22 Mar 2024: 9 Fe. b 20. 24. that localised sedimentary deposits of cosmic dust could have accumulated in aridenvironments on early Earth – in particular glacial settings that today producecryoconite sediments.
  8. 2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…

    https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf
    22 Mar 2024: Stapelfeldt ,22. Jordan M. Stone ,23 Jason J. Wang ,24, 25 Olivier Absil ,26 William O. ... MIRI Channel 4, Medium B 20.69 - 24.44 FULL FASTR1 1,680 – 1,770 1576.22.
  9. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: 1. Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. Corresponding author: Sascha P. Quanz, ETH Zurich, Institute for Particle Physics and Astrophysics, Zurich, Switzerland Contact
  10. MNRAS 000, 1–17 (2033) Preprint 19 June 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf
    22 Mar 2024: M = H(q)𝑇 N1H(q), (23). j = H𝑇 N1V. (24). Finally, I𝑠 = 𝝁 is used as the inferred brightness. ... 2). (27). This change to H(q) is used in Equations 21–24 or when comput-ing the model visibilities (Equation 18), with the code
  11. 2-nhb.dvi

    www.statslab.cam.ac.uk/~grg/books/hammfest/2-nhb.pdf
    22 Mar 2024: Journal of Applied Probability 24,809–826. Stout, W.F. (1974). Almost Sure Convergence.

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