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11 - 20 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. Flat Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/vircam_flatreport.html
    8 Dec 2006: 1.32 /- 0.05. 0.53 /- 0.01. 8. 2.23 /- 0.24. 0.61 /- 0.03. ... figure 5.10 Detector 10 (0.10%). figure 5.11 Detector 11 (0.24%). figure 5.12 Detector 12 (0.22%).

  3. Placing Our Solar System in Context:[A 12 step program ...

    https://people.ast.cam.ac.uk/~wyatt/mmeyer_etal_ppv.pdf
    19 Apr 2006: MIR.but more common around stars < 100 Myr. MIPS 24 um image of Vega disk. ... MIPS-24 MIPS-70. MIPS-160 JCMT-450CSO-350. HST. Do Stars with Inner Planets (< 5 AU) Also Have Kuiper Disks?

  4. ..............................................................…

    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.

  5. Pipeline CalibrationSimon Hodgkin(paper in prep) Outline • UKIRT…

    https://people.ast.cam.ac.uk/~wfcam/talks/hodgkin_ukidss_jul06.pdf
    3 Aug 2006: The observations span 05A and 05B, and comprise around 21 obs for the P272 field, and 24 for the P545 field.

  6. mnr9848.tex

    https://people.ast.cam.ac.uk/~wyatt/gfw05.pdf
    19 Apr 2006: This latter study is based on weak IRAS excesses,and four of the six systems identified with IRAS at 25 µm do nothave 24-µm excesses on re-examination by Spitzer

  7. mnr_7037.tex

    https://people.ast.cam.ac.uk/~wyatt/gw03.pdf
    19 Apr 2006: G8V 1HD 18757 22.9 G4V 2 Wide binaryHD 19373 10.5 G0V 1HD 20407 24.4 G3V 1HD 20766 12.1 G2V 2,‘B’ Wide binary (secondary)HD 20807 ... 1 G1V 2 Wide binary (primary); IRAS discHD 20619 24.7 G5V 1HD 20630 9.2 G5V 1 YoungHD 20794 6.1 G8V 1 ISO discHD

  8. Modeling the Structures of Dusty Disks: UnseenPlanets? Mark C. ...

    https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf
    19 Apr 2006: to the Sun, at about 23 AU, then migratedoutward to its current 30 AU orbit [24]. ... Sci., 27, 287–312 (1999).24. Malhotra, R., Astron. J., 110, 420–429 (1995).25.

  9. 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.

  10. PDF/48/aa5873-06.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf
    14 Dec 2006: 2 0.8 0.8 150 20 <1.9GJ 9809 M0 23 06 04.8 63 55 34 24.9 29.43 Loc Ass. ... 23 06 04.8 63 55 34 24.9 29.43 Loc Ass 0.5 7 0.36 2.2 2.2 7 26 <10.

  11. 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

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