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1 - 10 of 29 search results for katalk:za33 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. 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).

  3. 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.

  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 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.

  6. 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.

  7. 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.

  8. Submitted to ApJ, 3 January 2007, accepted 22 March ...

    https://people.ast.cam.ac.uk/~wyatt/wssr07.pdf
    23 Mar 2007: The 150t1age line delineatingthe upper envelope of the 24 µm detections (Rieke et al. ... 4.2.1. Sample of 46 A star disks detected at 24 and 70µm.

  9. 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.

  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. 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.

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