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  1. Results that match 1 of 2 words

  2. arX iv:0 704. 0873 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf
    18 Apr 2007: hot Jupiter –0.08 to 0.39 1.7–5 [500–1600] 70–200 1 % 2 1 %cool Jupiter –0.44 to 0.40 0.24–1.7 [75–500] ... 200 8 % 9 (5–11) %. planet & debris –0.13 to 0.27 0.10–0.24 [30–75] 5–30 5 % 3 1 %debris –0.52 to 0.18
  3. MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...

    https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf
    3 Jul 2007: 1), which fits the three longest wavelength fluxes, but cannotreproduce the 24 m flux. ... 1999, ApJ, 512, 377Hildebrand, R. 1983, QJRAS, 24, 267Holland, W. S., et al.
  4. https://people.ast.cam.ac.uk/~rgm/vhs/newsletter/VHS_Newsletter_1.txt

    https://people.ast.cam.ac.uk/~rgm/vhs/newsletter/VHS_Newsletter_1.txt
    19 Feb 2007: 24.1, 23.7, 23.3 and 22.6 respectively. ... respectively with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.
  5. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf
    5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)
  6. https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/summary.lis…

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/summary.list
    3 Sep 2007: 1.311 2001-06-07 21:23:46 24.08 J 0.97 1936.2 4.5 0.12 0.05 0.30 w_20010607_06523_sf_2 CIRSI_NGC135A ... 1.311 2001-06-08 05:12:43 24.01 J 0.97 1398.8 3.6 0.08 0.03 0.36.
  7. ESO Public Surveys Proposal Form Phase 1 Appendix B: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-response-final.pdf
    5 Jun 2007: The DESdesign reference survey strategy is to survey the full 5000deg2 in year 1 for 200secs per bandreaching 10sigma limits[AB mags] in g, r, i and z of 24.1, ... The goal for the full 5 years is a total exposure of 400, 400,1200, 2000 secs in g, r i
  8. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p1.pdf
    5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)
  9. arX iv:0 704. 3369 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf
    26 Apr 2007: 24). In Figure 4 we compare models having5 MJ between the planets with and without disc matter lo-cated inside the inner planet. ... The mass distributionfollows equation (24) and the outer disc mass is varied bychanging parameter Σ0out.
  10. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/wcg07.pdf
    18 Jul 2007: L. Arnold, F. Bouchy, C. Moutou (Paris: FrontierGroup), 24. Boss A., 2002, ApJ, 567, L149Butler R.
  11. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0_fjc.pdf
    5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)

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