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23 Nov 2007: ESO Survey Management Plan Form:VISTA Hemisphere Survey Phase 1. 1 The VISTA Hemisphere Survey SMP. PI: Richard McMahon, University of Cambridge, UK (rgm@ast.cam.ac.uk)Deputy/Co-PI: Andrew Lawrence, Institute for Astronomy, University of Edinburgh,

8 Nov 2007: Plans to perform direct FTP data transfer tests from JACH to CASU are also progressing and it is hoped to test this later in November. ... Camera Test data: The July Paranal engineering run produced 2,500 files which have been used for various tests (of

1 Nov 2007: CASU WFCAM/VISTA. External Links. Dafydd Wyn Evans (dwe @ ast.cam.ac.uk). Last modified: 1 Nov 2007.

10 Oct 2007: VISTA news - general news - cold camera test data report - letter to PIs [and ESO] 8. ... However, without further tests it is not clear if this will be the case.

5 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-.

18 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

3 Sep 2007: Example output. A night of pipeline-processed CIRSI data from the run on the INT has been used to perform a test-run of the scripts.

3 Sep 2007: A simple background gradient in an interleaved set of images was used to test the background subtraction. ... In particular, the tests ofand photometry show very similar results in both cases.

3 Sep 2007: For the initial tests, images from the INT wide field camera (WFC) were used. ... These were included on the plots. For the tests, only one CCD of the WFC is shown.

3 Sep 2007: Example output. A night of pipeline-processed CIRSI data from the run on the INT has been used to perform a test-run of the scripts.