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  2. Substructure searching — CSD Python API 3.1.0 documentation

    https://downloads.ccdc.cam.ac.uk/documentation/API/descriptive_docs/substructure_searching.html
    28 Mar 2024: Because this aromatic methoxy substructure is quite common in the CSD, we will limit our maximum number of hits to 200. ... ar_methoxy_hits = ar_methoxy_search.search(max_hit_structures=200, max_hits_per_structure=1) >>> len(ar_methoxy_hits) 200. To get
  3. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: 200. 0. 200. 400. µJy. /Bea. m. Figure 1. Naturally weighted ALMA 880𝜇m images of our BPMG M-dwarf sample. ... 0. 200. 400. µJy. /Bea. m. Figure 2. Naturally weighted ALMA 880𝜇m image of TYC 7443-1102-1.The stellar location is marked with a.
  4. Utilities — CSD Python API 3.1.0 documentation

    https://downloads.ccdc.cam.ac.uk/documentation/API/descriptive_docs/utilities.html
    28 Mar 2024: It may be populated by adding values:. >>> h.add_values([-1.0 0.01i for i in range(200)]) >>> print(h.frequencies) (10, 10, 10,. ).
  5. Draft version July 18, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 Mar 2024: collisional evolution. Only 6 systems with ages in the range 50 to 200 Myr were detected. ... The typical FWHM beam size of 1.′′5 (200 au) comfortably encompasses dust belts with radii up to 100 au.
  6. Editing molecules — CSD Python API 3.1.0 documentation

    https://downloads.ccdc.cam.ac.uk/documentation/API/descriptive_docs/molecule_editing.html
    28 Mar 2024: 3.669)) >>> a4 = Atom('C', coordinates=(-1.327, -3.345, 3.075)) >>> a5 = Atom('C', coordinates=( 0.200, -3.055, 2.977)) >>> a6 = Atom('C', coordinates=( 0.447, -1.874,
  7. DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/srw23.pdf
    22 Mar 2024: DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style in AASTeX631. Formation of Gaps in Self-gravitating Debris Disks by Secular Resonance in a Single-planet System. II. Towards aSelf-consistent Model. ANTRANIK A. SEFILIAN,1, 2 , ROMAN R.
  8. Draft version March 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: 6 Hull et al. 200 100 0 100 200Position along major axis (au).
  9. Release notes — CSD Python API 3.1.0 documentation

    https://downloads.ccdc.cam.ac.uk/documentation/API/release_notes.html
    28 Mar 2024: See Grids for details. the SQLite file distributed for use by the API contains over 200,000 entries that have anisotropic displacement parameters (ADPs), and nearly 2,000 further entries with
  10. MNRAS 000, 1–17 (2033) Preprint 19 June 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf
    22 Mar 2024: A case of a double Gaussian radial distribution, with = 0.03and 𝜎𝑟 = 20 au, peaking at 100 au and 200 au, shown in the middlepanel of Figure 2. • ... 0.06 0.08 0.10 0.12 0.14. h. 600. 500. 400. 300. 200.
  11. 22 Mar 2024: Astronomy & Astrophysics manuscript no. main ESO 2023October 11, 2023. Planetary system architectures with low-mass inner planets. Direct imaging exploration of mature systems beyond 1 au. C. Desgrange1,2, J. Milli1, G. Chauvin3, Th. Henning2, A.

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