Search

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.

5 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.

3 Sep 2007: Last updated: Tue Aug 19 14:24:15 2003.

3 Sep 2007: Last updated: Tue Aug 19 14:24:20 2003.

3 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.

24 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

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.

5 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

5 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.

5 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.

3 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.

18 Jun 2007: Steady-state evolution explains 24 and 70µm stats. Wyatt et al. (2007b).

23 Mar 2007: The 150t1age line delineatingthe upper envelope of the 24 µm detections (Rieke et al. ... 4.2.1. Sample of 46 A star disks detected at 24 and 70µm.

18 Apr 2007: hot Jupiter –0.08 to 0.39 1.7–5 [500–1600] 70–200 1 % 2 1 %cool Jupiter –0.44 to 0.40 0.24–1.7 [75–500] ... 200 8 % 9 (5–11) %. planet & debris –0.13 to 0.27 0.10–0.24 [30–75] 5–30 5 % 3 1 %debris –0.52 to 0.18

5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)

14 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

5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)

19 Feb 2007: 24.1, 23.7, 23.3 and 22.6 respectively. ... respectively with 10sigma limit of 24.6, 24.1, 24.3 and 23.9.

5 Jun 2007: To demonstrate the power of adding the VISTA IR data to the planned DESoptical data, we have constructed mock magnitude-limited galaxy samples (with 20 < i < 24 and redshifts0 < z < 2)

24 Apr 2007: stars at 24,70,160μm• Akari (2006-) currently doing all-sky survey 2-180μm• Herschel (2008-) observations at 60-670μm• Spica (2017+) planned 5-200μm. ... Structure is wavelength dependent!850μm. (Holland et al. 2006)24 and 70μm. (Su et al.