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https://people.ast.cam.ac.uk/~vasily/sdss/456/readme456.txt
https://people.ast.cam.ac.uk/~vasily/sdss/456/readme456.txt27 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 -
L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...
https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf19 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. -
Contents
https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/index.html17 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. -
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https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf19 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. -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html26 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). -
SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…
https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf19 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 -
Quasars and Galaxies at the Highest Redshifts
https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt8 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. -
mnr7957.tex
https://people.ast.cam.ac.uk/~wyatt/gwhd04.pdf19 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. -
Oxford Meeting
https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt15 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. -
Persistence Examples
https://people.ast.cam.ac.uk/~wfcam/docs/reports/persistence/persistence_examples.html26 May 2006: m. 20.3. s. 48 31' 40" and has a 2MASS J magnitude of 8.79. ... The individual frames are 20 second exposures taken in Z. About 20 seconds elapse from the end of 01867 and the start of 01868.
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