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Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/wcg07.pdf18 Jul 2007: L. Arnold, F. Bouchy, C. Moutou (Paris: FrontierGroup), 24. Boss A., 2002, ApJ, 567, L149Butler R. -
Data Flow System Document Title: VISTA Data Reduction Library ...
https://people.ast.cam.ac.uk/~wfcam/ukreview/VIS-SPE-IOA-20000-0010_latest.pdf7 Jun 2007: 23 2.16 Illumination Correction. 24. 3 Functional Description. 26 3.1 Recipes. ... 13 / kk leads to a relative area of. )41()31).(1( 222 rkrkrk ′′′ (2-24). -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070201.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_070201.txt14 Feb 2007: 21-24) and I am in the processes of dumping to disk the tapes with the fixed chips 1 & 2 hoping to get the remaining chips soon. ... Dec. 21-24). No data for 06B have been transferred yet to ESO because of the missing NDR data: it made sense to us to -
WFCAM simulations
https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made. -
WFCAM: DQC information for 20010607_sf
https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/dqc.html3 Sep 2007: Last updated: Tue Aug 19 14:24:20 2003. -
WFCAM: DQC information for 20010607
https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/dqc.html3 Sep 2007: Last updated: Tue Aug 19 14:24:15 2003. -
ESO Survey Management Plan Form:VISTA Hemisphere Survey Phase 1 ...
https://people.ast.cam.ac.uk/~rgm/vhs/smp/SMP_VHS_v1p1.pdf23 Nov 2007: ATLAS GPS21-22 DES ATLAS GPS22-23 DES ATLAS23-24 DES ATLAS. -
842 Publications of the Astronomical Society of the Pacific, ...
https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf18 Sep 2007: stellar luminosities. TheA stars (dark blue) are a sample of 46 detected at both 24 and 70mm (Wyattet al. ... A0, 3.6–24.8 pc for G0, and 1.8–8.6 pc for M0. -
arX iv:0 704. 3369 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf26 Apr 2007: 24). In Figure 4 we compare models having5 MJ between the planets with and without disc matter lo-cated inside the inner planet. ... The mass distributionfollows equation (24) and the outer disc mass is varied bychanging parameter Σ0out. -
WFCAM simulations
https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html3 Sep 2007: Passband. H. Magnitude zero-point. 24.8. Magnitudes. Sky brightness. 13.6. Mags/arcsec2. Magnitude limits. ... imcore_conf. only (Figure 23) and median magnitude difference (Figure 24) were made.
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