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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.

9 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.

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

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

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

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

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

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.

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: 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

22 May 2001: Tests of this method show that very fast warm of times may be achieved.

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.

10 Apr 2013: Section Unit Test Recipes.

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.

6 Nov 2006: Initially 120 square degrees are being released in order to test the system and receive comments. ... Tests are underway on the new baffling tube which should cut out remaining Moon glint problems.

9 Jan 2006: DWE generated some colour-colour plots from a crowded field (M17) to test the PSF-v-pipeline photometry (see item 7) 2. ... The list of demands is quite large and will take a considerable amount of work to implement and test.

18 Apr 2006: 7. VDFS VISTA update WJS reported that the telescope has passed the acceptance test, including (nearly all) the mirror supports. ... WJS said that he would pass this requirement on. WJS also added that the optical test camera has arrived in Edinburgh.

10 Mar 2005: MR has successfully finished the tests for the ESO code that pushes WFCAM data over to ESO. ... though more tests remain to be done. PH gave some useful comments regarding controllers for RAID arrays which may explain why apm6 is slow for multiple

29 Mar 2013: A few low-level (250m/s) interesting quirks have arisen in pipeline velocity comparison tests between different gratings e.g. ... MJI - que pasa con el v5 links STH - are the very red star tests for NB118 useful?

2 Feb 2006: The AIT3a tests are currently in progress. PSB was uncertain what the plans for the next few months were. ... He said that he would wait until the current batch of data has been processed and then test the algorithm on some real data (about end of January

5 Mar 2014: still playing catchup due to the upgraded security EGS - took pity and sent a text file of the latest VST and VISTA grades SC - system update tests on hold but in ... Slightly hidden from view WFCAM processing continues apace with a mix of normal astro

27 Sep 2011: EGS will find out if the EVALSO test transfers will recommence since getting more data more quickly would be useful here Upcoming: 27/06/11: the next VMC skypecon - will probably ... At some point, after yet more tests, this will require a re-run of all

26 May 2006: Tests were carried out using only LAS data, where the images are quite sparse, and the results were just as noisy, thus eliminating this explanation. ... In these tests, it was found that using the simple model and the decay characteristics measured above

12 Mar 2009: above. As part of the bug fix we also implemented, as an extended test for the 08B recataloguing, the mod to improve the Petrosian, Kron and Hall (PKH) radii and fluxes ... This data also provided a good independent test of the nebulosity filter

20 Nov 2023: 1. 2. Test particle evolution / secular resonancesThe orbits of test particles in a planetary system evolve due to the secular perturbations of planets whoseorbits also evolve due to their mutual perturbations. ... a) Consider a test particle in the two

14 May 2009: The tests carried out produced images with better resolution from the ground than have been obtained in space with the Hubble Space Telescope, and reached nearly 1000 times fainter than was

21 Apr 2009: STH will inquire about possibility/status of new WFCAM linearity measures when he goes out observing next week or so MJI forwarded UDS test results to JRL STH figured out the ... He has also being doing some extended mosaicing tests with MONTAGE which

10 Jun 2011: tests suggest (mostly) harmless 9. CASUHELPSs ------------- No corkers this month. ... JRL EGS JRL - sneakily attempt to get some VST data during 6th June meeting MJI - implement WFCAM astrometric fixes as revealed by GPS tests EGS - chew over the ESO

16 Jun 2015: It is convenient to be able to align and test the system during day-light and in all weather conditions. ... The tests were in two forms, long exposure conventional images were taken of the outputs of the beam combiner.

17 May 2005: In order to test transfer speed ING have been given an account on one of our PCs. ... MJI reported that he and JMI had done extensive I/O tests on the RAID file systems, the result being that all the CASU RAID EXT3 filestores (bar apm6_a) have

22 Oct 2011: The new server for VST, apm45, was spec'd, cost'd, ordr'd, delivr'd and installed and is rapidly filling up with assorted VST test data for ATLAS, VPHAS and ... To add to the pressure there will be a VPHAS meeting at the IoA November 14,15 to discuss the

5 Dec 2012: to twilights - hard to believe but needs following up with a few tests. ... To be continued. 9. Spectroscopic stuff ----------------------- Gaia-ESO the Gaia-ESO pipeline products velocity tests look good with sub-km/s accuracy.

28 Aug 2012: Tests on one night (20120104) where this problem happened with montonous regularity yield much improved results. ... 9. Spectroscopic stuff ----------------------- GaiaESO pipeline comparison test results look generally very good and there has even been

16 Jun 2015: Test this all as follows: SYS> archive [and watch the Talker to see if there is any errors. ... 00:00:00 00:00:00 test (must have colons) then use cirsi_grid.pl. Files will be created of the form name.gaia (ie test.gaia for the example above)

5 Dec 1998: CIRSI Overhead Timing tests. carried out on 03/04 Nov 1998 at 02am by rgm.

16 Jun 2015: test input catalogue file for cirsi_grid3.pl >you may need to edit this since I do not know the exact format of theDuPont Telescope Control System(TCS). ... type cirsi_grid3.pl DUPONT cirsi-test.cat cirsi-test.grid. This will generate some files

16 Jun 2015: test input catalogue file for cirsi_grid3.pl >you may need to edit this since I do not know the exact format of theDuPont Telescope Control System(TCS). ... type cirsi_grid3.pl DUPONT cirsi-test.cat cirsi-test.grid. This will generate some files

16 Jun 2015: The AAO selected a suitable bearing (originally intended for use with a radar tracker!) and conducted tests to verify that the axial runout specification is met by this precision bearing. ... At the IoA we have carried out stability tests of the complete

2 Nov 2006: In the following tests we have used the 2MASS PSC as the basis for all the astrometry. ... After a few tests it became clear that not only had we got the sign wrong in the predicted value for the distortion (easy to do) but also the magnitude of

26 Jan 2011: EGS will look at the impact of grouting on a sample of VVV data to extend these tests to more traumatic fields before we commit. ... With the grouting procedure in place, and assuming remaining tests go well, the plan is that all existing tile catalogues

6 Mar 2003: NB: this kind of thing is going in a different CDR doc concerning hardware: Tests between different locations in the UK in the day give sustained data transfers rates of 4 ... of positions in focus scan NFOCSCAN= 0 / Number of focus scans in focus test

One should check that all the exposures used are at the correct level (light level tests often mean the first few exposures are too high or too low).