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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 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

Index of /wfcam/docs. 2003-03-25 18:04. 75K. 2003-03-25 18:04. 846K. 2004-11-11 15:50. 154K. DigitalSignaturesPS.pdf. 2004-11-11 15:54. 79K. 2004-01-29 15:35. 4.7K. 2003-01-08 11:06. 247K. VDF-WFA-WSA-004-I2.html. 2003-09-23 12:19. 55K. 2003-12-08 09

Index of /vasily/sdss/orphan. 2009-01-29 12:15. 70K. 2009-01-29 12:15. 90K. 2009-01-29 12:15. -. 2009-01-29 12:15. 122K. 2009-01-29 12:15. 5.8K. 2009-01-29 12:15. 283K. 2009-01-29 12:15. 6.5K. 2009-01-29 12:15. 18K. 2009-01-29 12:15. 3.4K.

16 Feb 2004: available. While we can begin this process for WFCAM with laboratory test data, final tuning will require on-sky characterisation. ... Meanwhile we can use data from other infrared cameras to test various options.

Index of /vasily/data/catalogues. 2024-01-09 13:34. 32M. 2024-01-09 13:34. 2.3M. 2022-07-22 20:30. 478M. 2023-05-08 09:40. 24M. 2022-01-07 15:51. 7.4M. apogee_dr17_in_acc.fits. 2023-05-07 10:51. 1.0M. 2023-06-25 17:51. 8.4K. 2023-11-15 08:10. 2.9M.

Index of /vasily/sdss/stellar_halo. 2008-09-02 14:31. 66K. 2008-09-02 18:54. 185K. 2010-04-21 10:30. 555K. 2016-05-09 12:42. 745K. 2006-11-20 19:40. 29K. 2006-11-20 19:40. 29K. 2006-11-20 20:00. 1.0K. 2006-11-20 19:40. 111K. 2006-11-20 19:41. 136K.

9 Jan 2003: SJW to set up simulations to test parameter generation software, sensitivity to seeing etc. ... WFAU to do more tests to find bottleneck in network connectivity between Cambridge and Edinburgh.

8 Jan 2003: H:ukirtWFCAMDOCUMENTSActiveScience array tests.doc. Document Title Initial Science detector 41 test results. ... 6 of 13 H:ukirtWFCAMDOCUMENTSActiveScience array tests.doc. Test setupTests of Hawaii-2 #41 science detector were made in the test cryostat,

1 Mar 2011: WFCAM simulations - PSF and galaxy tests. 01-09-2003. 03-10-2003 [html]. ... VDF-TRE-IOA-00012-0001. Interleaving tests. 25-09-2003. 29-10-2004 [html].

16 Jun 2015: Reset correction test -- CNS verification of Pixcel online processing.

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

18 Dec 2002: Tests done on chips (one only): (a) Image persistence om (b) Crosstalk problem - but repeatable. ... d) Dark stability apparently ok. Test data: its proving difficult to get suitable test data eg.

21 Nov 2016: Tests. Applicants will be required to sit a one-hour non-calculator pre-interview test in mathematical skills during their interview visit. ... The tests will not be based on any particular syllabus and no past papers are available.

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

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.

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.

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

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

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.

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.

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.

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)

10 Apr 2013: int vircam_lincor_exec(cpl_plugin ) ; 00046 static int vircam_lincor_destroy(cpl_plugin ) ; 00047 static int vircam_lincor_test(cpl_parameterlist , cpl_frameset ) ; 00048 static int ... 00069 static int isfirst; 00070 static cpl_frame product_frame = NULL

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).

10 Apr 2013: create(cpl_plugin ); 00046 static int vircam_matchxy_exec(cpl_plugin ); 00047 static int vircam_matchxy_destroy(cpl_plugin ); 00048 static int vircam_matchxy_test(cpl_parameterlist , cpl_frameset ); 00049 static ... PAF / 00403 00404 if (vircam_paf_print(

6 Jul 2005: 30/09/2003. 01/09/2003. 3. End-to-end demonstration of operation of one mode in both ORACDR and CASU pipelines including comparitive tests of existing (Starlink-based) pipeline, the

18 Jan 2000: During the April 1998 commissioning period, test data on a small number of fields was obtained. ... This data is made available to the community. This test data is currently located in Cambridge, UK.

13 Dec 2002: Twilight, Sky, Dome - all have problems. STH doing tests. ROE also looking into dome flats (useful for pixel-to-pixel, something else used for vignetting).

13 May 2009: VIS-SPE-ATC-20500-0001. Interleaving tests. 25-09-2003. 29-10-2004 [html]. ... WFCAM simulations - PSF and galaxy tests. 01-09-2003. 03-10-2003 [html].

To circumvent the problem, one can suppress PGPLOT and write a test file to fit.txt be answering no to the question.

16 Jun 2015: Rachel Johnson <raj@ast.cam.ac.uk>. Last modified: Mon Nov 6 05:39:04 2000.

16 Oct 2003: CPU Run Times. Test case, downloading and running code as stands with different compilers, CPUs and Options.

10 Apr 2013: int vircam_matchstds_exec(cpl_plugin ); 00046 static int vircam_matchstds_destroy(cpl_plugin ); 00047 static int vircam_matchstds_test(cpl_parameterlist , cpl_frameset ); 00048 static int ... table outtab; 00069 } ps; 00070 00071 static int isfirst;

27 Nov 2003: test MEF data processed automated DQC monitoring tools developed using images and catalogues provisional pipeline progress monitoring tools with web interface programming completed for all basic modules ORAC-DR test routines ... Tests with ISAAC appear

19 Jun 2003: DWE has not obtained the data for the different seeing/offsets test of Ian Bond's software. ... DWE action to use WFC data to simulate undersampled offset data for interpolation and difference imaging tests is also ongoing.

16 Jun 2015: Note that the final value is mean rand(sd). Again this command is mostly used for generating test data.

29 Nov 1998: The magnitudes (and colours) are internally calibrated. Tests on the Northern catalogue show that the colours are consistent to /-0.2 magnitudes and the magnitude faint end zero-points are consistent

3 Aug 2003: The difficultly of defining quantitative tests to catagorize the 3 software packages was noted. ... DWE said that he had installed SWarp and was going to base the interpolation tests on this package since it incorporated all the well known methods.

12 Sep 2003: The following were comments regarding the document that were raised during the meeting: i No intrapixel sensitivity tests. ... work MJI provide feedback on VISTA IR detector test procedure document by the JRL end of the week.

18 Jul 2006: JRL reported that the ESO end-to-end test had been very successful. ... We supplied simulated data to test out our supplied V0.3 recipe modules.

27 Jul 2003: This is needed to do further tests of the pipeline monitoring and calibration scripts. ... Some example plots were shown and discussed and the list of tests discussed and some extra ones added.

16 Jun 2015: The results of the tests on astronomical objects and internal calibration sources are shown. ... The test observations produced in this chapter generally used most of the night to find and observe each star.

8 Jan 2004: STH checking the spatial systematics in the UFTI standards data and new test data is an ongoing task. ... A related issue is continuing to acquire laboratory test data and take part in assessing its characteristics.