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1 - 10 of 29 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 29 match some words.

  1. Results that match 1 of 2 words

  2. Estimate of the Number of CPU Nodes to Execute ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf
    29 Sep 2006: Data:. • Average of 200 Gb of science data per night (about 14 hours long). • ... Average night: 200 Gb/0.27 Gb = 740 images per night.

  3. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 Apr 2006: This 200-AU-sized regioncoincides with the slightly tilted inner disk identified optically withthe Hubble Space Telescope5. ... The possible relationship of these components has yetto be explored, but the lower inferred temperatures of the clumpparticles

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

    https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v3p0.pdf
    6 Jun 2006: Execute tiles that overlap with 200 deepest XMM pointings. • Fornax galaxy cluster(50deg2). ... The black filled circles are 200 deep public XMM pointings from the 2XMMcatalogue.

  5. Basic Debris Disk Model

    https://people.ast.cam.ac.uk/~wyatt/wyat06b.pdf
    21 Sep 2006: Dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al.

  6. PDF/36/aa3391-05.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/wyat05c.pdf
    19 Apr 2006: the range 110–200 AU with low eccentricitiesand inclinations (e < 0.01, I < 0.573). ... One problem is thatboth the 200 and 325 AU spirals have large azimuthal densityvariations which make them appear clumpy.

  7. SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…

    https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf
    19 Apr 2006: Accurate telescope pointing wascrucial to these observations and was checked before andafter each map using the nearby blazar 2255282 with rmserror of less than 200. ... Very littleinformation can be deduced about sizes or positions differ-ing by 200,

  8. VDFS UK VISTA User Requirements

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-SPE-IOA-00009-0001.pdf
    28 Sep 2006: Data Flow System. Document Title: UK VISTA User Requirements Document Number: VDF-SPE-IOA-00009-0001 Issue: 3.0 Date: 2005-07-05 Document Prepared by:. Will Sutherland (VISTA Project Scientist). Signature And date:. Document Approved by:. Jim

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

    https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf
    19 Apr 2006: 200 100 0 -100 -200RA offset, AU. -200. -100. 0. 100. ... 200. Dec. off. set,. AU. FIGURE 5. Impact of the outward migration of a Neptune mass planet on a planetesimal disk aroundVega [27]: orbital distribution of planetesimals at the beginning (top

  10. LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...

    https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf
    19 Apr 2006: Dust emissionpeaks are resolved with source sizes of 200 to 500 (1.7 104 to4.3 104 AU).

  11. VDF-WFA-VSA-004-I1.dvi

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-WFA-VSA-004-I1.pdf
    29 Sep 2006: VISTA DATA FLOW SYSTEM(VDFS). —————————–. for VISTA & WFCAM data. Pipeline / Science Archive Interface Control Document. authorN.C.Hambly (WFAU Edinburgh)Science Archive Project Scientist. numberVDF-WFA-VSA-004. issueDraft 1.0.

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