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1 - 20 of 28 search results for TALK:Vb20 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. 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:

  3. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html
    3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made.

  4. https://people.ast.cam.ac.uk/~rgm/vhs/v4/vdes-coi.log

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/vdes-coi.log
    5 Jun 2007: This is pdfeTeX, Version 3.141592-1.30.4-2.2 (Web2C 7.5.5) (format=pdflatex 2006.6.8) 28 JAN 2007 18:24 entering extended mode write18 enabled.

  5. WFCAM: DQC information for 20010607

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/dqc.html
    3 Sep 2007: Last updated: Tue Aug 19 14:24:15 2003.

  6. WFCAM: DQC information for 20010607_sf

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/dqc.html
    3 Sep 2007: Last updated: Tue Aug 19 14:24:20 2003.

  7. ESO Public Surveys Proposal Form Phase 1 Appendix B: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-Appendid-B-PSP-Response.pdf
    5 Jun 2007: The DES design referencesurvey strategy is to survey the full 5000deg2 in year 1 for 200secs per band reaching 10sigma limits[AB mags]in g, r, i and z of ... with 10sigma limit of24.6, 24.1, 24.3 and 23.9.

  8. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070201.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070201.txt
    14 Feb 2007: 21-24) and I am in the processes of dumping to disk the tapes with the fixed chips 1 & 2 hoping to get the remaining chips soon. ... Dec. 21-24). No data for 06B have been transferred yet to ESO because of the missing NDR data: it made sense to us to

  9. 842 Publications of the Astronomical Society of the Pacific, ...

    https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf
    18 Sep 2007: stellar luminosities. TheA stars (dark blue) are a sample of 46 detected at both 24 and 70mm (Wyattet al. ... A0, 3.6–24.8 pc for G0, and 1.8–8.6 pc for M0.

  10. Microsoft PowerPoint - wyattpub

    https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf
    24 Apr 2007: stars at 24,70,160μm• Akari (2006-) currently doing all-sky survey 2-180μm• Herschel (2008-) observations at 60-670μm• Spica (2017+) planned 5-200μm. ... Structure is wavelength dependent!850μm. (Holland et al. 2006)24 and 70μm. (Su et al.

  11. 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.

  12. 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.

  13. 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.

  14. 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)

  15. 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.

  16. 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)

  17. 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.

  18. 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

  19. 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)

  20. 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.

  21. 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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