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26 Jan 2006: These patterns are still being assessed, although a series of tests using a higher order r5 term showed some improvement. ... A series of tests using the UKIRT FS observations to monitor the WFCAM 2MASS calibration are being carried out, with very

19 Dec 2002: SJW to set up simulations to test parameter generation software, sensitivity to seeing etc. ... 13. CASU to forward prototype stacking and mosaicing software to WFAU for tests.

18 May 2018: To test out the design I made a scale model which could be used by my god-daughter's Barbie.

10 Feb 2003: Cambridge XMMSSC Internal pages. Test processing of XID work.

19 Mar 2003: asap what other UKIRT?WFCAM test data do we need? - more flats (dome cf. ... SJW to set up simulations to test parameter generation software, sensitivity to seeing etc.

24 Feb 2005: For this test we generated catalogues of objects on all four detectors from each observation.

10 Dec 2004: 5 Speed of code. While carrying out these tests, the processing speed was noted in comparison with. ... However, tests on optical data show that these improvements may not be realized.

10 Jul 2003: It will then be off, so that CASU can process and test the pipeline. ... Detector tests are needed to verify these effects.) SJW thought that the crosstalk was high.

24 Mar 2010: The generic flatfield test data we would like to acquire prior to WFCAM commissioning. ... Eckhard is doing further tests to find the source of the Cambridge-Edinburgh bottleneck.

23 Jan 2003: asap what other UKIRT?WFCAM test data do we need? - more flats (dome cf. ... SJW to set up simulations to test parameter generation software, sensitivity to seeing etc.

1 Jul 1999: This algorithm can be used to look at the statistics of stellar distributions and was applied to the Bright Star Catalogue to test our theory of stellar evolution and to constrain

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

16 Jun 2015: CIRPASS test observations from Cambridge. We have attached the CIRPASS IFU to an 8 inch telescope in Cambridge to test instrument performance.

6 Dec 2004: 5 Analysis. The first tests were carried out using perfect, rather than measured, PSFs. ... 6 Crowded field tests. Tests were also carried out on the effectiveness of PSF fitting in crowded regions.

22 Oct 2003: When this is not available during engineering tests, this may be a fixed value;. • ... NFOC = 0 / Number of positions in focus scan. NFOCSCAN= 0 / Number of focus scans in focus test.

14 Mar 1999: Linearity tests using sequences of dome flats revealed CCD#2 and CCD#4 to have significant non-linearities over the whole dynamic range.

29 Jan 2004: Wo Mark Casali's report on science array tests actions02.html Me Actions from last year actions02.txt (early version of above) campipehardware.html Sy Pipeline layout (hardware and software)

8 Jul 2000: Background ED Event Designator EDH EPIC Data Handling Unit EDAC Error Detection and Correction EDU Event Detection Unit EDU EPIC Data Handling Unit EE End-to-End [Test] Einstein Einstein Observatory ... Support Equipment GSFC Goddard Space Flight Centre

round($x),"y"=>round($y)); } if(empty($long))$long = 202.015; if(empty($lat)) $lat = 33.556; $im = imagecreatefrompng("fos_dr6.png"); $red = imagecolorallocate ($im, 255,0,0); $scale_x = imagesx($im); $scale_y = imagesy($im); $pt = getlocationcoords(

20 Aug 2003: WFCAM ON-SKY CHARACTERIZATION TESTS. A. Adamson, P. Hirst (JAC)M. Irwin, D. ... Tests of different flat fielding algorithms.7. Assess flatfield stability (impacts on data taking and reduction strategy).