Search

Search Funnelback University

Search powered by Funnelback
10 results 20 results 50 results
Relevance Date (Newest first) Date (Oldest first) Title (A-Z) Title (Z-A) Distance URL (A-Z) URL (Z-A) Shuffle
Did you mean pc524 |u:people.ast.cam.ac.uk?
11 - 20 of 21 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 21 match some words.

  1. Results that match 1 of 2 words

  2. Astronomy & Astrophysics manuscript no. aa ©ESO 2024April 9, ...

    https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf
    9 Apr 2024: 2016)found a significant warm excess at 24 µm of Spitzer/MIPS basedon the Dodson-Robinson et al. ... The beam size is represented by a white ellipse (left: 2.24′′ 1.84′′, middle: 2.28′′ 1.89′′, right: 1.43′′ 1.12′′) inthe

  3. Cosmic dust fertilization of glacial prebiotic chemistry on early ...

    https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf
    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.

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

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: 1HD 9672 01:34:38 -15:40:34 5.61 5.53 A1V 406 57.08 1HD 10472 01:40:24 -60:59:56 7.61 6.69 F2IV/V 307 ... 409 45.60 1HD 14082B 02:17:25 28:44:30 7.74 6.36 G2V 219 39.75 1AG-Tri 02:27:29 30:58:24 10.12 7.24

  5. 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

  6. Astronomy & Astrophysics manuscript no. main ©ESO 2023October 11, …

    https://people.ast.cam.ac.uk/~wyatt/dmch23.pdf
    22 Mar 2024: 0613. 3920. 18-1. 1-24. H23. HD. 9949. 220. 18-0. 2-03. H23. ... BD. 0613. 3920. 18-1. 1-24. H23. HD. 9949. 220. 18-0. 2-03.

  7. 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

  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. DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/srw23.pdf
    22 Mar 2024: Equations (24)–(27). 4 A. A. SEFILIAN, R. R. RAFIKOV, & M.

  10. MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/hwd22.pdf
    22 Mar 2024: MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled usingMNRASLATEXstyle file v3.0. Has the dust clump in the debris disk of Beta Pictoris moved? Y.Han,1 M.C.Wyatt,1 W.R. F.Dent,21Institute of Astronomy, University of Cambridge, Madingley Road

  11. 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

Refine your results

clear all

Date

Search history

Recently clicked results

Recently clicked results

Your click history is empty.

Recent searches

Recent searches

Your search history is empty.