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1 - 10 of 57 search results for watson |u:people.ast.cam.ac.uk

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  2. Mark Wyatt

    https://people.ast.cam.ac.uk/~wyatt/
    15 Apr 2024: Mark Wyatt. My research mostly focusses on the formation and evolution of stars and their planetary systems. In particular I am interested in the dusty debris material that surrounds some stars, including the Sun, during their main sequence phase.

  3. https://people.ast.cam.ac.uk/~xmmssc/xid/wfc_bynight.txt

    https://people.ast.cam.ac.uk/~xmmssc/xid/wfc_bynight.txt
    17 Nov 2005: 3:PATT-XID:Y:Y /data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.080/0.004/0.016/17:./lplogs/20000725.int:: ... 26:3:PATT-XID:Y:Y

  4. https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/wfc_bynight.txt

    https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/wfc_bynight.txt
    19 Feb 2003: data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.080/0.004/0.016/17:a href=./lplogs/20000725.int:: ... Y:Y /data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.095/0.005/0.022/18:a href=./lplogs/20000726.int::

  5. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.pdf
    5 Jun 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.

  6. 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.

  7. arX iv:1 004. 0644 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/sw10.pdf
    6 Apr 2010: arX. iv:1. 004. 0644. v1 [. astr. o-ph. EP. ] 5. Apr. 201. 0Astronomy & Astrophysicsmanuscript no. astars˙3rd c ESO 2010April 6, 2010. Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. Wyatt2. 1 Astrophysics Group,

  8. 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.

  9. https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt

    https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt
    16 Jun 2015: Spot a 00:47:33.410 -25:17:13.6 Spot i 00:47:33.013 -25:17:18.12 Spot n 00:47:33.063 -25:17:17.20

  10. ESO Survey Management Plan Form:VISTA Hemisphere Survey Phase 1 ...

    https://people.ast.cam.ac.uk/~rgm/vhs/smp/SMP_VHS_v1p1.pdf
    23 Nov 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.

  11. Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…

    https://people.ast.cam.ac.uk/~wyatt/swd08.pdf
    29 Apr 2008: Astronomy & Astrophysicsmanuscript no. 8719 c ESO 2008April 28, 2008. The Nature of Mid-Infrared Excesses From Hot Dust AroundSun-like Stars. R. Smith1,2, M. C. Wyatt1, and W.R.F. Dent3. 1 Institute of Astronomy, University of Cambridge, Madingley

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