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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. -
https://people.ast.cam.ac.uk/~rgm/vhs/v4/vdes-coi.log
https://people.ast.cam.ac.uk/~rgm/vhs/v4/vdes-coi.log5 Jun 2007: This is pdfeTeX, Version 3.141592-1.30.4-2.2 (Web2C 7.5.5) (format=pdflatex 2006.6.8) 28 JAN 2007 18:24 entering extended mode write18 enabled. -
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. -
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. -
https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/summary.lis…
https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/stack/summary.list3 Sep 2007: 1.311 2001-06-07 21:23:46 24.08 J 0.97 1936.2 4.5 0.12 0.05 0.30 w_20010607_06523_sf_2 CIRSI_NGC135A ... 1.311 2001-06-08 05:12:43 24.01 J 0.97 1398.8 3.6 0.08 0.03 0.36. -
Basic Debris Disk Model
https://people.ast.cam.ac.uk/~wyatt/wyatt_uf07.pdf24 Apr 2007: 2005):. F 24/. F. Steady-state planetesimal belt evolution. The size distribution in a collisionalcascade is to first order described by a power law. ... Wyatt et al. (2007a). This model accurately reproduces the fraction of stars in different age bins -
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. -
ESO Public Surveys Proposal Form Phase 1 Appendix B: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-response-final.pdf5 Jun 2007: The DESdesign reference survey strategy is to survey the full 5000deg2 in year 1 for 200secs per bandreaching 10sigma limits[AB mags] in g, r, i and z of 24.1, ... The goal for the full 5 years is a total exposure of 400, 400,1200, 2000 secs in g, r i -
ESO Public Surveys Proposal Form Phase 1 Appendix B: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-Appendid-B-PSP-Response.pdf5 Jun 2007: The DES design referencesurvey strategy is to survey the full 5000deg2 in year 1 for 200secs per band reaching 10sigma limits[AB mags]in g, r, i and z of ... with 10sigma limit of24.6, 24.1, 24.3 and 23.9. -
MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...
https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf3 Jul 2007: 1), which fits the three longest wavelength fluxes, but cannotreproduce the 24 m flux. ... 1999, ApJ, 512, 377Hildebrand, R. 1983, QJRAS, 24, 267Holland, W. S., et al.
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