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  1. Results that match 1 of 2 words

  2. SPIRAL phase A: A prototype IFS for the AAT

    https://people.ast.cam.ac.uk/~optics/spiral/papers/spie.htm
    16 Jun 2015: The objectives of the phase-A study are to develop the construction techniques for a new type of fibre-fed spectrograph and to test it on the AAT by carrying out
  3. VIRCAM Pipeline: VIRCAM Data Reduction Pipeline Manual

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/
    10 Apr 2013: Section Unit Test Recipes.
  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100421.txt
    5 May 2010: There's enough high latitude data to do overlap tests. Should be ready by next meeting. ... Various transfer tests between Santiago and Garching have been made to tune system performance and further tests including to Cambridge are planned.
  5. Night Sky Brightness at Cerro Pachon

    https://people.ast.cam.ac.uk/~rgm/vista/site/pachon_sky/
    12 Jul 1999: The model calculates V magnitude light output at zenith. Since the street light are all Sodium and there are virtually no Mercury lamps, the V band is a good test case.
  6. Rockwell PICNIC array

    https://people.ast.cam.ac.uk/~optics/tech/hawaii/picnic.htm
    16 Jun 2015: We currently have one NICMOS science grade array for COHSI along with a test device, we are waiting for the delivery of the second science grade device to make up the
  7. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt
    19 Dec 2011: There was much discussion of observing strategy and the results from the test data taken so far (any choice bits are incorporated in the VST section). ... image tests, require much more effort to characterise and attempt to find solutions for.
  8. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100324.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100324.txt
    19 Apr 2010: are written and prototyped in different languages (toolkit and pipeline) and the result intercompared, test datasets are also used to check results when bug fixing or smaller upgrades occur. ... Direct tests revealed no problems! but a more indirect
  9. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130327.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130327.txt
    19 Apr 2013: He will investigate if any suitable VVV field test data has been taken. ... There was (to us at least) an amusing phone call from an old pal in the detector division at ESO regarding their recent discovery, during some instrument tests, of stripes due
  10. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120829.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120829.txt
    4 Sep 2012: This has been upgraded to use double precision in the inversion and an extra iteration and now produces sub-mas precision in forward-backward transformation tests. ... test. So far so good, but even better is to observe complete tiles for shallow surveys.
  11. Minutes of VISTA Camera Calibration Meeting

    https://people.ast.cam.ac.uk/~wfcam/docs/camera_calibration_meeting.html
    17 Mar 2004: Some discussion on whether pipeline astrometric calibrations can feedback into the pointing tests as well as guide star feedback. ... No new templates would be needed. This calibration would update data obtained from the laboratory tests.

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