Search
Search Funnelback University
- Refined by:
- Date: 2007
1 -
10 of
29
search results for TALK:ZA31 24 / |u:people.ast.cam.ac.uk
where 0
match all words and 29
match some words.
Results that match 1 of 2 words
-
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/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 -
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-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. -
wyatt
https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf18 Jun 2007: Steady-state evolution explains 24 and 70µm stats. Wyatt et al. (2007b). -
ESO Public Surveys Proposal Form Phase 1 Title: The ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2-Appendix-B-PSP-Response.pdf5 Jun 2007: ESO Public Surveys Proposal Form Phase 1. reaching 10sigma limits[AB mags] in g, r, i and z of 24.1, 23.7, 23.3 and 22.6 respectively. ... with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
Recent searches
Your search history is empty.