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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. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060612.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060612.txt
    18 Jul 2006: The latter is contingent on final tests on the updated verification and flagging procedure (see later). ... It was noted again that some Cambridge presence at these tests would be desirable.

  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. CASU analysis of SV data for WFCAM

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

  5. 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

  6. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_061101.txt
    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.

  7. 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

  8. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060919.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060919.txt
    1 Oct 2006: A finder telescope will be installed in November/December for telescope and dome tests. ... PSB said that he visited RAL last Tuesday (12th) and took part in acquiring further VIRCAM test data.

  9. Document Title: VISTA Infra Red Camera Calibration Plan Document ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0002.pdf
    28 Sep 2006: We will be using 2MASS as the primary astrometry calibrator and in tests on similar mosaic instruments we have shown that our suggested ZPN distortion model, combined with a linear plate ... This will be characterised through laboratory tests during

  10. arX iv:a stro -ph/ 0504 086 v1 4 A ...

    https://people.ast.cam.ac.uk/~wyatt/srms05.pdf
    19 Apr 2006: To test the sensitivity of the model fits to the assump-tion of astronomical silicates, we also fit the radial pro-files using amorphous carbon grains (ρ = 1.85 ... grains. TheMIPS and SCUBA observations are then distinctly dif-ferent grain populations.

  11. Calibration of WFCAM data from 2MASS: an investiga-tion and ...

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/2masscal_old.pdf
    6 Jan 2006: Tests using a larger aperture (4 arcsecond diameter) for the calculationof the zeropoint show no difference. ... We think this is an important test of the 2MASS-based calibration.

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