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11 - 20 of 28 search results for katalk:za33 24 |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. ESO Public Surveys Proposal Form Phase 1 Title: The ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2-Appendix-B-PSP-Response.pdf
    5 Jun 2007: ESO Public Surveys Proposal Form Phase 1. reaching 10sigma limits[AB mags] in g, r, i and z of 24.1, 23.7, 23.3 and 22.6 respectively. ... with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.

  3. 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.

  4. 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: 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)

  5. WFCAM Catalogues Document Number: VDF-SPE-IOA-00009-0001 Version 4…

    https://people.ast.cam.ac.uk/~rgm/vhs/smp/WFCAM-catalogues-v4p0.pdf
    19 May 2007: 24 arcsec diameter45 Error in flux The aperture fluxes can be combined with later-derived aperture.

  6. 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)

  7. 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.

  8. Basic Debris Disk Model

    https://people.ast.cam.ac.uk/~wyatt/wyatt_uf07.pdf
    24 Apr 2007: 2005):. F 24/. F. Steady-state planetesimal belt evolution. The size distribution in a collisionalcascade is to first order described by a power law. ... Wyatt et al. (2007a). This model accurately reproduces the fraction of stars in different age bins

  9. 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)

  10. hd113766_dust_25Sep2007

    https://people.ast.cam.ac.uk/~wyatt/lcwm08.pdf
    5 Oct 2007: excess 24 and 70 µm flux. In their follow-on study, which provided the data used in this work,. ... silicate emission features at 9.8, 11.2, 16.2, 19, 24, and 34 µm.

  11. https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/summary.list

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/summary.list
    3 Sep 2007: 1.311 2001-06-08 01:08:24 24.07 J 0.81 1450.9 7.5 0.21 0.11 0.25 w_20010607_06614_2 1637-046B ... 1.311 2001-06-08 01:08:24 24.07 J 0.96 1588.9 8.1 0.17 0.11 0.28 w_20010607_06614_3 1637-046B

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