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https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070221.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070221.txt28 Feb 2007: Although this problem is expected to be negligible for VISTA WJS has been asked to get this included in the list of integration tests. ... comments on above to STH WJS add field rotation flat field tests to integration tests JRL find out more about -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0_fjc.pdf5 Jun 2007: veys as a test bed for the VISTA infrared surveys, and which is sufficiently flexible as to be applicable to anyimaging survey project requiring an end-to-end (instrument to -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/wcg07.pdf18 Jul 2007: 3.4 Observational tests. Here we suggest three observational tests of the critical solidmass model:. ... Observational tests of the model includea flattening of the metallicity relation for Z > 0.5 dex andalso a flattening as planet searches continue. -
arX iv:0 704. 0873 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf18 Apr 2007: We aim to test whether one underlyingproperty has a highly significant effect on the outcome, andso intentionally ignore other properties that could affect theplanetary system formed around an individual star. ... 2003;Sozzetti 2004); a K-S test here -
842 Publications of the Astronomical Society of the Pacific, ...
https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf18 Sep 2007: 2004), and these comprise a significantlybiased data set. With the SUNS survey data, it will be possible to test forplanetary system evolution. ... The survey will test the applicability of the solar systemitself. One model for the origin of debris disks -
Data Flow System Document Title: VISTA Data Reduction Library ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010_latest.pdf7 Jun 2007: 1.8 2007-06-05 All Undated all references to dfs tags. Expanded descriptions of test recipes to include output data. ... 109 8.2 Recipe (plugin) Tests. 115. 9 Development Plan. 116 10 Appendix: QC1 Parameters. -
SMP_VHS_RIXES_All_Responses_v1p0
https://people.ast.cam.ac.uk/~rgm/vhs/smp/SMP_VHS_RIXES_All_Responses_v1p0.pdf24 May 2007: science. 3. As part of their quality control tests, the survey team expects to test the galaxy-star. -
Microsoft PowerPoint - wyattpub
https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf24 Apr 2007: be used to test models. … -
hd113766_dust_25Sep2007
https://people.ast.cam.ac.uk/~wyatt/lcwm08.pdf5 Oct 2007: ured fluxes by a best-fit blackbody (with a value of Tgr = 490K found from χ2 minimization test-. ... As a test of the robustness of our best-. 18. fit model, the last column in Table 1 also gives the best-fitting χ2ν found after deleting a particu-. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.pdf5 Jun 2007: The VDFS is aworking systems-engineered system that is already being successfully employed for the UKIRT WFCAM sur-veys as a test bed for the VISTA infrared surveys, and which is
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