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1 - 10 of 29 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 29 match some words.

  1. Results that match 1 of 2 words

  2. 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.

  3. 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.

  4. 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.

  5. 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.

  6. 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

  7. 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

  8. WFCAM simulations

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/
    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.

  9. 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.

  10. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 Jun 2007: Steady-state evolution explains 24 and 70µm stats. Wyatt et al. (2007b).

  11. 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.

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