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21 - 30 of 74 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 74 match some words.

  1. Results that match 1 of 2 words

  2. L187 The Astrophysical Journal, 619:L187–L190, 2005 February 1� 2005. …

    https://people.ast.cam.ac.uk/~wyatt/ghwd05.pdf
    19 Apr 2006: Dominik,5 and H. J. Walker6. Received 2004 September 17; accepted 2004 December 20; published 2005 January 10. ... The total dust flux within a diameter circle is′1 37.0mJy at 850mm and mJy at 450mm, in good2.5 250 20.

  3. L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...

    https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf
    19 Apr 2006: The diameter of theP.A. = 1757 5 107major axis of the emission at 10.8 mm is 20.2, which corre-sponds to 215 AU. ... At 18.2 mm the maximum extent of theemission is 20.0 (198 AU), which is about 90% the size ofthe 10 mm emission.

  4. https://people.ast.cam.ac.uk/~vasily/sdss/456/readme456.txt

    https://people.ast.cam.ac.uk/~vasily/sdss/456/readme456.txt
    27 Jun 2006: The resulting distance moduli are: dmag = [18.2, 20.9, 16.8] In principle, from the CMD matching, you can't really shift the ridgeline by more than 0.05 mag

  5. Contents

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/index.html
    17 Jan 2006: A reasonable estimate to account for this is that the 2x2 plots need to be adjusted by 20% (ie. ... However, one of the frames exhibited a large magnitude term in y amounting to 0.05 pixel (20 mas) over the observed magnitude range.

  6. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 Apr 2006: wing along lines through the star. The nine evenly spaced contour levels are at the 10, 20,. ... We ignore results for the regionwithin 20 AU of the star because of the contribution of the silicate feature and uncertaintiesin the PSF.

  7. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html
    26 Jan 2006: The images mimic fuzzy looking galaxies and in this image peak at typically 5-20 counts above sky. ... measured using a conventional method) is therefore also 1.20 (Parseval's Theorem and power spectrum <-- FT --> autocorrelation).

  8. SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…

    https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf
    19 Apr 2006: Received 2002 April 17; accepted 2002 September 20. ABSTRACT. New submillimeter images of the cold dust emission around the nearby main-sequence star Fomalhaut arepresented. ... mJy beam1). Integrated Fluxb. (mJy). 450. 7.1, 12.3 119 20 7.4, 16.2 124 20

  9. Quasars and Galaxies at the Highest Redshifts

    https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt
    8 Mar 2006: 4400. 22.1. 2.6. V. 5500. 21.3. 3.5. R. 6000. 20.4. 3.9. ... 3000. 22.0. 21.2. 20.0. 19.5. 100. Galactic Plane Magellanic Clouds. 1500.

  10. mnr7957.tex

    https://people.ast.cam.ac.uk/~wyatt/gwhd04.pdf
    19 Apr 2006: Combining this with the beam size, the effectiveresolution is 20 arcsec or 70 au. ... Figure 1. 850-µm image of τ Ceti, smoothed to 20-arcsec resolution.

  11. Oxford Meeting

    https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt
    15 Apr 2006: 0.10. V. 5500. 21.3. 21.4. 9.6. 3.5. 0.15. R. 6000. 20.4. ... In some the star–formation at this level may have begun at z10-20.

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