Search

6 Jun 2006: Execute tiles that overlap with 200 deepest XMM pointings. • Fornax galaxy cluster(50deg2). ... The black filled circles are 200 deep public XMM pointings from the 2XMMcatalogue.

28 Sep 2006: Data Flow System. Document Title: UK VISTA User Requirements Document Number: VDF-SPE-IOA-00009-0001 Issue: 3.0 Date: 2005-07-05 Document Prepared by:. Will Sutherland (VISTA Project Scientist). Signature And date:. Document Approved by:. Jim

29 Sep 2006: VISTA DATA FLOW SYSTEM(VDFS). —————————–. for VISTA & WFCAM data. Pipeline / Science Archive Interface Control Document. authorN.C.Hambly (WFAU Edinburgh)Science Archive Project Scientist. numberVDF-WFA-VSA-004. issueDraft 1.0.

29 Sep 2006: Data:. • Average of 200 Gb of science data per night (about 14 hours long). • ... Average night: 200 Gb/0.27 Gb = 740 images per night.

28 Sep 2006: event that observations of a secondary photometric standard field with a density of 100-200 objects per detector are available, then the illumination correction can be measured by looking at the

28 Sep 2006: Data Flow System Document Title: VISTA Data Reduction Library Design Document Number: VIS-SPE-IOA-20000-0010 Issue: 1.5 Date: 2006-09-28 Document Prepared by:. Jim Lewis Peter Bunclark Simon Hodgkin (CASU). Signature and Date:. Document Approved by:.

28 Nov 2006: 2004; Kim et al.2005), have conducted photometric surveys of about 200 nearbystars at 24 and 70m.

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=

19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the

19 Apr 2006: Including only dwarf stars, about 200 disccandidates remain. However, some of these are very young starsstill in the pre-main-sequence phase, which still possess primordialdiscs.