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  2. WFCAM Catalogues Document Number: VDF-SPE-IOA-00009-0001 Version 5…

    https://people.ast.cam.ac.uk/~wfcam/docs/catalogues.pdf
    2 Sep 2008: 24 arcsec diameter45 Error in flux The aperture fluxes can be combined with later-derived aperture.
  3. Change Record

    https://people.ast.cam.ac.uk/~wfcam/docs/jul2007_linearity.doc
    20 Jan 2008: 2-24. 0.1. 6. 1.67. 0.04. 2-32. 0.3. 7. 0.96. 0.03. 2-33. ... 10. 0.69. 0.07. 1-27. 0.3. 11. 1.49. 0.04. 1-24. 0.3. 12.
  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080429.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080429.txt
    1 May 2008: 24 hours of it being taken.
  5. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080623.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_080623.txt
    27 Jun 2008: As noted previously this has generally resulted in observed nights of raw WFCAM data being available on disk here roughly 24 hours after the data is taken. ... It is checked, ingested and read to go for processing roughly another 24 hours later.
  6. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_081127.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_081127.txt
    16 Dec 2008: The raw data arrives and is checked, MEF'd and ingested within 24 hours of it being taken.
  7. 7009.pmd

    https://people.ast.cam.ac.uk/~wyatt/mwmt08.pdf
    1 Feb 2008: Because the clearing time of dust in the 24-µm-emitting zone (10–60 AU) is 1–10 m.y. ... HD 69830 is a three-planet systemwith a strong 24-µm excess (see section 4) (Beichman etal., 2005b).
  8. arX iv:0 812. 2475 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/pfwb08.pdf
    17 Dec 2008: 3.47F(iii) 700 1 No No 24 49 3 0 11 13 0.27 3.97F(iv) 100 1 No No 44 34 1 1 9 11 0.30
  9. arX iv:0 810. 5087 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf
    3 Nov 2008: Modelling indicates that the extension arises from an edge-on disk of radius0.5 arcsec ( 24 AU).
  10. 29 Apr 2008: 3.1.1. TIMMI2. The observations on TIMMI2 were taken over three runs on 11-12 September 2003, 19-21 November 2003 and 24-26 January2005 (proposals 71.C-0312, ... 123356d G1V O(0.1)e 20.9 14+ 1270 (53) 3 615 (56)128400 G5V 0.3i 20.4 260+ 178 (24) 61+ 64
  11. Dynamics of small bodies in planetary systems Mark C. ...

    https://people.ast.cam.ac.uk/~wyatt/wyat08.pdf
    8 Jul 2008: Rather the dust distribution seen at 24 and 70 µm extendsout to 800 AU [73]. ... Wyatt. Eridani disk which is a narrow ring at 60 AU with a well resolved inner hole[24].

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