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Estimate of the Number of CPU Nodes to Execute ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf29 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. -
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https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf19 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 -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v3p0.pdf6 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. -
Basic Debris Disk Model
https://people.ast.cam.ac.uk/~wyatt/wyat06b.pdf21 Sep 2006: Dense rings at 200 and 325 AU with tightly wound spiral structure (Clampin et al. -
PDF/36/aa3391-05.pdf.url
https://people.ast.cam.ac.uk/~wyatt/wyat05c.pdf19 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. -
SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…
https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf19 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, -
VDFS UK VISTA User Requirements
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-SPE-IOA-00009-0001.pdf28 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 -
Modeling the Structures of Dusty Disks: UnseenPlanets? Mark C. ...
https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf19 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 -
LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...
https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf19 Apr 2006: Dust emissionpeaks are resolved with source sizes of 200 to 500 (1.7 104 to4.3 104 AU). -
VDF-WFA-VSA-004-I1.dvi
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-WFA-VSA-004-I1.pdf29 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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