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1 - 10 of 42 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 42 match some words.

  1. Results that match 1 of 2 words

  2. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 Apr 2006: Corresponding peak. signal-to-noise ratios are 27, 48, 24 and 15, respectively. ... We used thestandard g Reticulum to determine the PSF at 24.6 mm.

  3. 58419 1321..1340

    https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf
    19 Apr 2006: Crosses show the location of a planetesimal in the different resonances (2 : 1, 5 : 3, 3 : 2, and 4 : 3,from top to bottom) at intervals of 1/24 of the ... l1:24. e0:42. ; ð33Þ. D5 :3h i 13:2 þ 290:0=l1:33. ; ð34Þ.

  4. aa2073.dvi

    https://people.ast.cam.ac.uk/~wyatt/wyat05b.pdf
    19 Apr 2006: A&A 433, 1007–1012 (2005)DOI: 10.1051/0004-6361:20042073c ESO 2005. Astronomy&. Astrophysics. The insignificance of P-R drag in detectableextrasolar planetesimal belts. M. C. Wyatt. UK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9

  5. arX iv:a stro -ph/ 0311 593 v1 26 N ...

    https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf
    19 Apr 2006: 32 0.02 0.13 0.04 < 0.5HD207129 0.60 0.03 0.15 0.02 0.31 0.04 < 0.24. ... However, sub-mm observations made withSCUBA on the JCMT indicate a diameter of 24 3 arc-sec (Holland et al.

  6. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: 6 Su et al. Fig. 9.— Radial dependent [24][70] distribution for the Vegadisk. ... To produce the observed [24][70]color, additional components must be invoked. 4.4.

  7. arX iv:a stro -ph/ 0601 592 v1 26 J ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/hewettetal.pdf
    28 Sep 2006: 4.162 2.130 5.626 2.349 -0.529 -0.117 -0.293 0.074 0.105 24.4 2 8.5 283 3.57. ... 4.190 0.301 2.457 1.409 -0.147 0.092 -0.288 0.074 0.132 14.6 10 8.0 859 4.24.

  8. arX iv:a stro -ph/ 0603 608 v2 1 Se ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/dye.pdf
    28 Sep 2006: 35 K multiple 20.8. J multiple 24.8UDS 0.77 H multiple 23.8. ... SFA 04:30,25:00 ZY JHK cen. 24. Orion SFA 05:29,02:36 ZY JHK cen.

  9. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html
    26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7.

  10. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/
    26 Jan 2006: 24.2 [using an average gain of 5.1 = 4.3 after correcting for intrapixel capacitance] UFTI (e-/s) ---- ---- 24.5 24.7 24.2. ... 9.0 4.2 5.80 24.4 #4 49.1 4.4 5.17 22.7.

  11. CASU analysis of WFCAM commissioning data - I

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/index.html
    2 Nov 2006: Z Y J H K Overall zero-point (count/s) 22.8 22.7 23.0 23.4 22.6 WFCAM (e-/s) 24.4 24.3 24.6 25.0 ... 24.2 [assumes above gain measures ok] UFTI (e-/s) ---- ---- 24.5 24.7 24.2.

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