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  1. Results that match 1 of 2 words

  2. Persistence

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/persistence/
    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
  3. CASU analysis of WFCAM commissioning data - I

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/
    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
  4. Flat Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/
    8 Dec 2006: Figure 1.16 Detector 16. 2. Self Flat Correction. As a first test for the repeatability of the flats, we flat corrected each of the 10s flats that went into the ... 0.49 /- 0.01. 16. 2.45 /- 0.11. 0.65 /- 0.01. In order to test whether the linearity
  5. Flat Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_flatreport/vircam_flatreport.html
    8 Dec 2006: Figure 1.16 Detector 16. 2. Self Flat Correction. As a first test for the repeatability of the flats, we flat corrected each of the 10s flats that went into the ... 0.49 /- 0.01. 16. 2.45 /- 0.11. 0.65 /- 0.01. In order to test whether the linearity
  6. Dark Exposure Properties of VIRCAM Detectors

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/vircam_darkreport/vircam_darkreport.html
    21 Oct 2006: Figure 51. Detector 16. 6. Readnoise and Gain. The data that were taken as part of the AIT included flats that were meant to be part of the tests for linearity.
  7. mnr9848.tex

    https://people.ast.cam.ac.uk/~wyatt/gfw05.pdf
    19 Apr 2006: A Kolmogorov–Smirnov test showsa probability of only P = 0.6 per cent that the debris and planetstars have the same metallicity distribution. ... of the system that doesaffect the presence of detectable debris remains to be determined.Better statistics
  8. Estimate of the Number of CPU Nodes to Execute ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf
    29 Sep 2006: We have used 6 processors to run this test on the main science recipe, using 12 input raw framesand creating 21 products. ... The detailed processing time of this test is:. recipe time = 320 seconds ( 20% for missing functionalities).
  9. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060510.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060510.txt
    15 May 2006: Comments on WFAU minutes PSB reported on the current round of transfer tests. ... The camera all-up tests will start shortly and the camera is cooling down.
  10. On the calibration of WFCAM data from 2MASS Authors: ...

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/2masscal.pdf
    29 Sep 2006: 5 Internal consistancy of the photometry. A simple way to test the homogneneity of the photometric calibration is to look at thedispersion in the median colours of high galactic latitude WFCAM
  11. Dust_in_the_Debris_Disk_Around_HD69830_09Nov2006

    https://people.ast.cam.ac.uk/~wyatt/lbbw07.pdf
    16 Nov 2006: level (Figure 1). As a test of the data reduction, we re-reduced the IRS data using the S13. ... As a test of the robustness of our best. fit model, the last column in Table 1 also gives the best-fitting χ2ν found after deleting a.

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