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1 - 5 of 5 search results for watson |u:people.ast.cam.ac.uk

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  2. ApJ409619o.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwcm11.pdf
    23 Feb 2012: was performed, with 1 cycle of 6 s integration at eachposition (Watson et al.

  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120829.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120829.txt
    4 Sep 2012: Watson Varricat came up with an interesting problem relating to WFCAM and crowded field photometry, e.g.

  4. ms_v2.dvi

    https://people.ast.cam.ac.uk/~wyatt/rcmw12.pdf
    22 May 2012: H., Sheehan, P., Watson, D. M., Manoj, P., & Najita, J.

  5. Observing Kepler stars with WISE

    https://people.ast.cam.ac.uk/~wyatt/kw12.pdf
    7 Jul 2012: arX. iv:1. 207. 0521. v1 [. astr. o-ph. EP. ] 2. Jul 2. 012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 5 July 2012 (MN LATEX style file v2.2). Confusion limited surveys: using WISE to quantify the rarit y ofwarm dust around Kepler stars.

  6. The Astrophysical Journal, 701:2019–2032, 2009 August 20…

    https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf
    1 Aug 2012: 2004). In order to avoid time-consuming peak-up, theobservatory was operated in IRS spectral mapping mode wherea 2 3 raster (spatial dispersion) centered on the star wasperformed (Watson et al.

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