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1 - 10 of 42 search results for TALK:Vb20 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. 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.

  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt
    9 Aug 2006: 3. Report from VDMT MJI and STH attended the VDMT meeting in Edinburgh on 24 July. ... MJI reported on the main points: The UK review of VDFS will be held in Cambridge on 24/25 October.

  4. 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%).

  5. 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

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

    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.

  7. 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.

  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. ESO Public Surveys Proposal Form Phase 1 Title: The ...

    https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v4p2-Appendix-B-PSP-Response.pdf
    9 Oct 2006: ESO Public Surveys Proposal Form Phase 1. reaching 10sigma limits[AB mags] in g, r, i and z of 24.1, 23.7, 23.3 and 22.6 respectively. ... with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.

  10. 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?

  11. SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...

    https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf
    19 Apr 2006: The total measured flux was 1:51 0:24 Jy (S=N 7);the dominant uncertainty in this flux estimate is the calibrationuncertainty.

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