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1 - 10 of 45 search results for Economics test |u:people.ast.cam.ac.uk where 0 match all words and 45 match some words.

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  2. VDFS UK VISTA User Requirements

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-SPE-IOA-00009-0001.pdf
    28 Sep 2006: Cf [RD05] Sec 4.8. Comment: This enables mapping of photometry vs position on the focal plane, which can test (for example) residual gradients due to scattered light, varying aperture correction

  3. VDF-WFA-VSA-004-I1.dvi

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-WFA-VSA-004-I1.pdf
    29 Sep 2006: NFOC = 0 / Number of positions in focus scan. NFOCSCAN= 0 / Number of focus scans in focus test.

  4. Ufti Flatfielding Test Data Requirements

    https://people.ast.cam.ac.uk/~wfcam/testdata.html
    26 May 2006: UFTI Flatfielding Test Data. We want to use UFTI test data to get a better handle on the flat field properties of the array/telescope system, and investigate the various contributions

  5. THE ASTROPHYSICAL JOURNAL, 527 : 918È944, 1999 December 20The ...

    https://people.ast.cam.ac.uk/~wyatt/wdtf99.pdf
    19 Apr 2006: THE ASTROPHYSICAL JOURNAL, 527 : 918È944, 1999 December 20The American Astronomical Society. All rights reserved. Printed in U.S.A.(1999. HOW OBSERVATIONS OF CIRCUMSTELLAR DISK ASYMMETRIES CAN REVEAL HIDDEN PLANETS :. PERICENTER GLOW AND ITS

  6. PSF Fitting of WFCAM Data: Tests on realdata Document ...

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf3/psf3.pdf
    17 Jan 2006: 5 Large-scale production tests 6. 6 UDS test 6. 7 Crowded field tests 10. ... 7 Crowded field tests. Tests have been carried out using data covering M17 in order to test the performance in more crowdedfields.

  7. Persistence

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/persistence/index.html
    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

  8. 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

  9. 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

  10. NEW DEBRIS DISKS AROUND NEARBY MAIN-SEQUENCE STARS:IMPACT ON THE ...

    https://people.ast.cam.ac.uk/~wyatt/bbsg06.pdf
    28 Nov 2006: 3.3. Detection of 70 m Excess. Having used 24 m fluxes to test the accuracy of our stellarphotosphere predictions, we next consider the frequency andstrength of excess emission at 70

  11. Mon. Not. R. Astron. Soc. 334, 589–607 (2002) Collisional ...

    https://people.ast.cam.ac.uk/~wyatt/wd02.pdf
    19 Apr 2006: However, it is difficult to test thishypothesis as the proposed planets are not detectable with currenttechniques, and such interpretations must be treated with cautionuntil alternative explanations have been explored. ... 2002) could be collisional in

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