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11 - 20 of 42 search results for KaKaoTalk:ZA31 24 24 |u:people.ast.cam.ac.uk where 0 match all words and 42 match some words.

  1. Results that match 2 of 3 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. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt
    6 Nov 2006: The UK VDFS review was held on 24/25 October at Cambridge.

  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060105.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060105.txt
    9 Jan 2006: The last GANTT chart we have says 24 March, but it is unclear if this is the current target date.

  5. ..............................................................…

    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.

  6. 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?

  7. 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.

  8. 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.

  9. 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

  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. NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE ...

    https://people.ast.cam.ac.uk/~wyatt/bbsg06.pdf
    28 Nov 2006: a Significance of 24 m excess (eq. [1]).b Significance of 70 m excess (eq. ... 2000). Finally,HD 23249 and HD 55892 have 2 < 24 < 3 and 70 < 2.

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