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19 Dec 2011: in the interim he released the processed VST test data to the ATLAS and VPHAS PIs via a simple passwd-protected web page - ongoing ALL - progressed as much as possible all ... There will be a VPHAS meeting here at the IoA November 14-15 to discuss among

6 Mar 2013: A l'autre main a good benchmark/null result for the next test. ... However, es ist noch nicht klar and we await the red star test results with something approaching interest.

30 Nov 2009: This has all been processed to the pawprint level. Tiling tests are still ongoing using the SV data as a scapegoat for different strategies. ... Detailed tests projecting the residuals onto the detector grid reveal no measureable wavelength dependence of

7 Jun 2009: MJI sorting out the VISTA i/o disks is on hold until the GAIA team finish assorted i/o tests on the new RAID system. ... MJI asked about the progress with the tiling software, tests with MONTAGE, and in particular what the contents of the tile FITS

11 Apr 2011: EGS - checked the EVALSO test file internet transfers from ESO Garching to AKY Cambridge and found that for the month of data under consideration a total of 8 files were missing ... We also heard news that the VST test camera is on and delivering Image

4 Nov 2013: Part of the reason we made the cataloguing code available was for people to do exactly these sort of tests. ... Fortunately EGS had kept a copy of the phase3 deliverables (well almost, it did include a bunch of undelivered "test depth" images and conf

4 Feb 2005: This 2 Tbytes of data resides on RAID disks and has been used as the basis for a series of tests. ... Sky Flats and Fringing ---------------------- Preliminary results from tests on flats show them to be stable over a period of a few nights.

16 Jun 2015: FITS writing code which must be distributed and operated before 1999-01-01 should be coded to test the current year to decide whether to use the old date format or

28 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

24 Jul 2012: SC will contact network support downtown and see if they can shed some light since all internal tests here reveal nothing wrong. ... 9. Spectroscopic stuff ----------------------- GaiaESO pipeline tests e.g. derived velocities, are looking good and the

16 Jun 2015: The objectives of the phase-A study are to develop the construction techniques for a new type of fibre-fed spectrograph and to test it on the AAT by carrying out

10 Apr 2013: Section Unit Test Recipes.

5 May 2010: There's enough high latitude data to do overlap tests. Should be ready by next meeting. ... Various transfer tests between Santiago and Garching have been made to tune system performance and further tests including to Cambridge are planned.

12 Jul 1999: The model calculates V magnitude light output at zenith. Since the street light are all Sodium and there are virtually no Mercury lamps, the V band is a good test case.

16 Jun 2015: We currently have one NICMOS science grade array for COHSI along with a test device, we are waiting for the delivery of the second science grade device to make up the

19 Dec 2011: There was much discussion of observing strategy and the results from the test data taken so far (any choice bits are incorporated in the VST section). ... image tests, require much more effort to characterise and attempt to find solutions for.

19 Apr 2010: are written and prototyped in different languages (toolkit and pipeline) and the result intercompared, test datasets are also used to check results when bug fixing or smaller upgrades occur. ... Direct tests revealed no problems! but a more indirect

19 Apr 2013: He will investigate if any suitable VVV field test data has been taken. ... There was (to us at least) an amusing phone call from an old pal in the detector division at ESO regarding their recent discovery, during some instrument tests, of stripes due

4 Sep 2012: This has been upgraded to use double precision in the inversion and an extra iteration and now produces sub-mas precision in forward-backward transformation tests. ... test. So far so good, but even better is to observe complete tiles for shallow surveys.

17 Mar 2004: Some discussion on whether pipeline astrometric calibrations can feedback into the pointing tests as well as guide star feedback. ... No new templates would be needed. This calibration would update data obtained from the laboratory tests.