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11 - 20 of 28 search results for katalk:Vb20 808 |u:people.ast.cam.ac.uk where 0 match all words and 28 match some words.

  1. Results that match 1 of 2 words

  2. MNRAS 000, 1–11 (2018) Preprint 27 June 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/sbbc18.pdf
    31 Jul 2018: The four com-parison stars are TYC 3162-1320-1, 3162-808-1, 3162-1001-1, and 3162-1073-1, with B values of 12.133, 12.382, 11.721,and ... The useablecomparison stars are TYC 3162-808-1 (AAVSO 118) andTYC 3162-1001-1 (AAVSO 113).

  3. Draft version March 10, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/edhm20.pdf
    10 Mar 2020: Draft version March 10, 2020Typeset using LATEX twocolumn style in AASTeX62. The HOSTS survey for exozodiacal dust: Observational results from the complete survey. Ertel, S.,1, 2 Defrère, D.,3 Hinz, P.,2 Mennesson, B.,4 Kennedy, G. M.,5 Danchi, W.

  4. MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/aght19.pdf
    17 Jan 2020: MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled using MNRAS LATEX style file v3.0. Are Inner Disc Misalignments Common? ALMA Reveals an IsotropicOuter Disc Inclination Distribution for Young Dipper Stars. M. Ansdell,1,2,3? E. Gaidos,4 C.

  5. Draft version April 5, 2018Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mmkw18.pdf
    5 Apr 2018: Draft version April 5, 2018Typeset using LATEX twocolumn style in AASTeX61. AN EMPIRICAL PLANETESIMAL BELT RADIUS - STELLAR LUMINOSITY RELATION. L. Matrà,1, S. Marino,2 G. M. Kennedy,3 M. C. Wyatt,2 K. I. Öberg,1 and D. J. Wilner1.

  6. https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_h20_absorption…

    https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_h20_absorption.txt
    16 Jun 2015: 0.9547 0.9342 0.9147 0.8962 0.8785 807. 0.9281 0.9038 0.8803 0.8588 0.8388 808.

  7. MNRAS 000, 1–13 (2018) Preprint 23 August 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/irgm18.pdf
    23 Aug 2018: c 2018 The Authors. arX. iv:1. 808. 0732. 0v1. [as. tro-.

  8. The Development of High-Resolution Imaging in Radio Astronomy

    https://people.ast.cam.ac.uk/~bothwell/Files/annurev.astro.39.1.457.pdf
    28 Jul 2021: 26 Jul 2001 13:43 AR AR137H-12.tex AR137H-12.SGM ARv2(2001/05/10)P1: GSR. Annu. Rev. Astron. Astrophys. 2001. 39:457–509. THE DEVELOPMENT OF HIGH-RESOLUTIONIMAGING IN RADIO ASTRONOMY. K. I. KellermannNational Radio Astronomy Observatory,

  9. arX iv:0 911. 3426 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/pgdm09.pdf
    19 Nov 2009: arX. iv:0. 911. 3426. v1 [. astr. o-ph. SR. ] 1. 8 N. ov 2. 009. Mon. Not. R. Astron. Soc. 000, 1–? (2009) Printed 19 November 2009 (MN LATEX style file v2.2). Target selection for the SUNS and DEBRIS surveys for. debris discs in the solar

  10. Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …

    https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf
    18 Apr 2022: Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED ESO 2022April 11, 2022. Large Interferometer For Exoplanets (LIFE):. I. Improved exoplanet detection yield estimates for a large mid-infraredspace-interferometer mission. S.P. Quanz1,

  11. arX iv:a stro -ph/ 0311 593 v1 26 N ...

    https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf
    19 Apr 2006: 0.74 808.9 60.

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