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21 - 30 of 72 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 72 match some words.

  1. Results that match 1 of 2 words

  2. UFTI Service Observation Reductions

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/ufti_service/index.html
    16 Feb 2004: f20030923_00312. The lower lefthand quadrant shows the most worrying trend. These features do decay with time though and return to near normal within 10 to 20 minutes.

  3. 1 Introduction

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/psf/
    6 Dec 2004: could also be accounted for (the detection limit is about J=20 [Irwin 2003]).

  4. https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/obsplan/20041224/al…

    https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/obsplan/20041224/almanacs/20041224.al
    10 Dec 2004: GST Moonset : 7 20 GST Moon at civil midnight: illuminated fraction 0.975 1.6 days until full moon, RA and dec: 4 56 21, 26 13.6 The sun is

  5. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_040210.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_040210.txt
    12 Feb 2004: WJS is drafting a first version of this. MJI have discussed dome flats for VISTA with WJS and confirmed that 10-20% PSB variation in illumination across the array was fine. ... MJI showed some images of raw data (6x20s coadd); the same dark-corrected

  6. 1 Introduction

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/interpol/
    26 Mar 2004: Transformation. Shift/pixels. x. y. 1. 0.05. 0.10. 2. 0.15. 0.20. 3.

  7. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_041103.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_041103.txt
    5 Nov 2004: 3rd November 2004 Hoyle committee meeting room 10.00 - 13:20 (inc. ... It will then remain on until 20 June. The following WFCAM run will be 15 August until the end of 2005.

  8. Minutes of VISTA Camera Calibration Meeting

    https://people.ast.cam.ac.uk/~wfcam/docs/camera_calibration_meeting.html
    17 Mar 2004: Detector Characteristics (NNB) Three engineering detectors have been tested #15 Large defect (bad pixels) 10-20% of chip Bands seen - different to plots shown at FDR - was this due to scaling ... Non-linearity is 1.9% (over 20-80% range) QE 59% 57% 49% J

  9. https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/camxid/nps_pos1/txt/x…

    https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/camxid/nps_pos1/txt/xwc_outcome.txt
    15 Sep 2004: 23.75 0 3 11 X0011 16 53 21.42 14 20 36.5 0.3 1.7e02 3.1e-14 0.84 -0.30 -0.53 0.22 Y ... wfc1 16 53 21.38 14 20 38.7 2.4 0.7 -2.3 3.0e00 0.67 22.30 -3 20.84 -2 22.99 1 22.84 -2

  10. https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/camxid/MBM12/txt/xwc_…

    https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/camxid/MBM12/txt/xwc_outcome.txt
    15 Sep 2004: 60 -1 17.30 -1 17.47 -3 -23.73 0 3 24 X0024 02 55 20.88 19 24 45.9 1.2 4.8e01 1.3e-14 0.87 ... 0.31 -0.28 NaN Y X0024_wfc1 02 55 20.91 19 24 48.4 2.4 -0.4 -2.4 1.4e02 0.00 18.83 -3 18.30

  11. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_041020.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_041020.txt
    4 Nov 2004: He also reported that he has written some 20 observing recipes for the commissioning run.

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