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VDFS UK VISTA User Requirements
https://people.ast.cam.ac.uk/~wfcam/ukreview/VDF-SPE-IOA-00009-0001.pdf28 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. -
THE ASTROPHYSICAL JOURNAL, 527 : 918È944, 1999 December 20The ...
https://people.ast.cam.ac.uk/~wyatt/wdtf99.pdf19 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. -
Document Title: VISTA Infra Red Camera Calibration Plan Document ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0002.pdf28 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, -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060628.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060628.txt18 Jul 2006: 3. Report on VISTA PSP meeting JRL reported on the VISTA PSP meeting he attended in Edinburgh on 20 June. -
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https://people.ast.cam.ac.uk/~wyatt/dgdj01.pdf19 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= -
Data Flow System Document Title: VISTA Data Reduction Library ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010.pdf28 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. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060308.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060308.txt11 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 -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060126.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060126.txt2 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 -
Placing Our Solar System in Context:[A 12 step program ...
https://people.ast.cam.ac.uk/~wyatt/mmeyer_etal_ppv.pdf19 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. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060510.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060510.txt15 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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