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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: Date: 05/07/2005 Issue: 3.0 Page: Page 20 of 33 Author: W. ... 1350 GB/night of observing. One exposure per 20 sec for 13 hours i.e.
  3. THE ASTROPHYSICAL JOURNAL, 527 : 918È944, 1999 December 20The ...

    https://people.ast.cam.ac.uk/~wyatt/wdtf99.pdf
    19 Apr 2006: e@ (1 [ b)1Je2 ] 2be cos f ] b2 , (20)u8 @ [ u8 f [ f @ arctan [b sin f/(b cos f ] e)]. ... 21). Analysis of equations (19), (20), and (21) shows that theorbits of the largest fragments, those for which b 0.1, aresimilar to that of the parent.
  4. 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: 20 4.1 Purpose. 20 4.2 Reset Frames. 22 4.3 Dark Frames. ... issue 1.0, 2001-03-28 [RD4] VISTA Infrared Camera Technical Specification, VIS-SPE-ATC-06000-0004,. issue 2.0, 2003-11-20 [RD5] VISTA IR Camera Software Functional Specification,
  5. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060628.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060628.txt
    18 Jul 2006: 3. Report on VISTA PSP meeting JRL reported on the VISTA PSP meeting he attended in Edinburgh on 20 June.
  6. 19 Apr 2006: "$# %&('). ,.-0/21436587$9;:<3=?>A@0B+CDFE!3GH+?I JK=?@ML,-N/FONDF:!-0/2GH31P:Q9;:!RS=?TU-MV0DWXRU>AGH+.-ZY,-5X-N=.-N>"-0/2[,D I2@M>"-0]Y29;Y29;E!3IU@X3MCD_X+?36UI23/8Y29UEa@N=B+?3/Sb0-0>AFc6d e0DUfg-N=BbihK92jk5X-NBml. Cno/2GHp,36=?]BGHq5@Mrs7)1H@0=
  7. Data Flow System Document Title: VISTA Data Reduction Library ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010.pdf
    28 Sep 2006: 78 6.17 vircam_persist. 79 6.18 vircam_photcal. 81 6.19 vircam_platesol. 83 6.20 vircam_sky_flat_combine. ... jk. kjjjj CIII , (2-20). Doc: VIS-SPE-IOA-20000-0010 Issue: 1.5 Date: 2006-09-28.
  8. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060308.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060308.txt
    11 Mar 2006: The split seems to be 80:20 between CASU and SEGUE. Note that the CASU part includes ESO as well as WFAU transfers. ... There is still a need for assessing how serious a problem it is and RGM said that he will use a list of 1000 known spurious outliers
  9. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060126.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060126.txt
    2 Feb 2006: In a nutshell, data up to 31 December has been processed and checked, up to 20 October has been transfered by WFAU and up to 25 October has been transfered to
  10. Placing Our Solar System in Context:[A 12 step program ...

    https://people.ast.cam.ac.uk/~wyatt/mmeyer_etal_ppv.pdf
    19 Apr 2006: this meeting). MIR. Step #7. Cool Debris Disks (< 100 K) are Common (10-20 %) around Sun-like Stars. ... 2005),Hillenbrand et al. 2006. 30+- 10 Myr45 to? AU1x10-7 Msun. 700+- 300 Myr 20 to <100 AU6.9x10-8 Msun.
  11. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060510.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060510.txt
    15 May 2006: About 20 of these overlap WFCAM data. These are well-calibrated photometric fields which will help with WFCAM photometric calibration issues including the next topic. ... There will be a meeting for VISTA Public Surveys in Edinburgh on 20/21 June and RGM

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