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3 Sep 2007: 21.15. 0.121. 1525. 2. 20.97. 20.98. 0.136. 1698. 3. 21.10. 21.09.

3 Sep 2007: 21.15. 0.121. 1525. 2. 20.97. 20.98. 0.136. 1698. 3. 21.10. 21.09.

3 Sep 2007: Passband. Measured 5-sigma limiting magnitude. Magnitude at 50% completeness. Z. 20.8. ... Software. 5-sigma limiting magnitude. Magnitude at 50% completeness. artdata. 20.00. 19.9.

22 Jul 2007: Sky brightness: The median values are 20.30, 20.22 and 20.09. Sky noise: Fractional Sigma of Sky Value Distribution, expressed as magnitude. ... The photometric zeropoint distributions are very similar. SEGUE p05 has a similar sky brightness to DR6 with

5 Jun 2007: 20 v1.0o Standard LaTeX Graphics (DPC,SPQR) (/usr/local/teTeX/share/texmf.local/tex/latex/graphics/trig.sty Package: trig 1999/03/16 v1.09 sin cos tan (DPC) ) ... words of font info for 20 fonts, out of 2000000 for 2000 58 hyphenation exceptions out of

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

5 Jun 2007: From fjc@ieec.fcr.es Tue Oct 3 20:44:41 2006 Date: Tue, 3 Oct 2006 14:17:37 0200 (CEST) From: Francisco Javier Castander fjc@ieec.fcr.es To:

3 Sep 2007: Passband. Measured 5-sigma limiting magnitude. Magnitude at 50% completeness. Z. 20.8. ... Software. 5-sigma limiting magnitude. Magnitude at 50% completeness. artdata. 20.00. 19.9.

5 Jun 2007: 20 v1.0o Standard LaTeX Graphics (DPC,SPQR) (/usr/local/teTex/share/texmf.local/tex/latex/graphics/trig.sty Package: trig 1999/03/16 v1.09 sin cos tan (DPC) ) ... DECam.png. /focalplane.png] [19] [20] AED: last page setting LastPage [21]

5 Jun 2007: The proposed VHS survey will have a 10σ limit in Y of 20.4[Vega]; see Table 1. ... The Y-Z>1.5 constraintfor Y=20.4 corresponds to a Z limit of 21.5(5σ).

23 Nov 2007: VIKING, VVV, VMC) will result in coverage of the whole southern celestialhemisphere (20,000deg2) to a depth 4 magnitudes fainter than 2MASS/DENIS in at least two wavebandsJ and Ks. ... 10 ATLAS GPS10-11 ATLAS GPS11-12 ATLAS GPS12-13 ATLAS GPS13-14 ATLAS

23 Mar 2007: Mmax =. (. 3.8 106ρr3.5(dr/r)DcM 0.5? tage. ). (. (12q 20)[1 1.25(e/I)2]0.5(18 9q)G(q, Xc). ). , ... 1-5 (diamond=small excess),. 5-20 (square=medium excess), > 20 (triangle=large excess).

18 Jun 2007: While the test took 20 days using a single-thread Sybase system, the Kognitio system took 8 minutes! ... WFCAM news MR said that processing was complete up to 20 April except for a small chunk of January data that is still being processed.

16 May 2007: 18 4.3 Triage. 19 4.4 Software. 20 4.5 Hardware. 21. 4.5.1 Processing Power. ... Doc: VIS-SPE-IOA-20000-0017 Issue: 1.1 Date: 2007-05-08. VISTA Data Flow. System. Cambridge Reduction and Analysis Pipeline Page: 20 of 23.

28 Feb 2007: ADASS 2007 - update 8. AOB - NAM (Preston, April 16-20) - EURO-VO - Kavli update - CPL workshop Minutes ------- 1. ... This was the case. MJI also asked if there was any interest in attending NAM (Preston, April 16-20).

5 Jun 2007: 1.0 19.4(20.3) 20.2(21.1) 20.7(21.6) 0.94 10.0. ... UKIDSS LAS uses SDSS z’ with a median 5σ limit(Vega) of 20.3.

7 Jun 2007: 81 6.20 vircam_platesol. 83. 7 Data Reduction CPL Plugins. 86 7.1 vircam_reset_combine. ... jk. kjjjj CIII , (2-20). where jI is the observed frame and jI′ the corrected version.

17 Apr 2007: AOB - conference proceedings for ESO workshop - cass38 resurrects yet again - NAM (Preston, April 16-20) - rolling grant application Minutes ------- 1. ... It has now gone off-line for hopefully the final time. NAM (Preston, April 16-20): MJI asked who

8 Feb 2007: Processing Wide-Field Imaging data. Mike Irwin. N4244 confidence map stack 20 dithered i-band frames. ... SB. Seeing. Ellipticity. MJD - 50000. N5466 r’-band. IPHAS = 7500x2 GP fields 20 < l < 220 -5 < b < 5.

5 Jun 2007: ESO-VISAS (visas@eso.org) Version 3.1; Printed October 3, 2006 22:20 page 1 of 21. ... ESO-VISAS (visas@eso.org) Version 3.1; Printed October 3, 2006 22:20 page 3 of 21.

5 Oct 2007: from within 20, 50, and 80 AU, respectively, of HD113766A. Including data obtained from the. ... 20. optically thin but highly extended disk of Beta Pic, (Chen et al.

18 Feb 2007: VIKING, VVV, VMC) will result in coverage of the whole southern celestialhemisphere (20,000deg2) to a depth 4 magnitudes fainter than 2MASS/DENIS in at least two wavebandsJ and Ks. ... Because of potential variables we ideally wish to get at least two

14 Feb 2007: 20 - Chip 2 for: Oct. 26 - Nov. 27 "At the moment I've MEFed all the complete new data (Dec.

9 Aug 2007: ING: The duplicate CDs and DAT tapes are being skipped and should make enough room in the CASU storeroom to accommodate the remainder of the CDs still in Room 20 in

31 Jan 2007: There are about 20 runs in total. 6. WFCAM news No data has been received yet.

10 Oct 2007: Keys are held by RWA, MR and Mark Hurn. Requests for the oldest (20 years old) ING data have almost dried up - 19 over the last 6 months and 4 in

19 Feb 2007: K(AB;5sigma)=21.3 (5) VHS (PI: McMahon) [20,000 JK, K(AB:5sigma)=20.0, ZY over reduced area] (6) A single ultra-deep field (merger of Dunlop, Franx, ... The original proposal was a 7 year program with over 20,000deg2 with | | exposure times of 180, 180,

30 Apr 2007: MR said that, ignoring data before 20 December and the incomplete 6 nights in January, only a few more nights of 06B (up to 31st March) data remain to be processed.

7 Feb 2007: Dark-time: J-band. skyJ=16.11 mag σJ=0.38 mag N=1343. Dark-time: H band. skyH=14.20 mag σH=0.29 mag N=1824.

3 Sep 2007: 1.311 2001-06-07 23:20:46 24.01 J 1.02 1798.3 4.3 0.12 0.05 0.28 w_20010607_06568_sf_2 CIRSI_NGC133B ... 1.311 2001-06-07 23:20:46 24.01 J 1.02 1922.9 4.5 0.10 0.04 0.26 w_20010607_06568_sf_3 CIRSI_NGC133B

18 Jun 2007: Late heavy bombardment model of (Gomes et al. 2005). 20. Conclusions 1 (Good news)Most disk radial structure explained by steady-state evolution of aplanetesimal belt due to collisions and radiation

18 Apr 2007: 2005) findinga range from 72/1330 = 5.4 % within 5 AU up to an extrap-olation of 11 % within 20 AU. ... 2005, e.g) need a fewtimes the Minimum Mass Solar Nebula, which comprised ap-proximately 20 MJ up (Davis 2005).

5 Jun 2007: Response: The original VHS proposal was a 7 year program which aimed to survey the full 20,000deg2 ofsouthern celestial hemisphere with exposure times of 180, 180, 60, 60 seconds in

19 May 2007: 20 Aperture flux 1 These are a series of different radii soft-edged apertures designed toadequately sample the curve-of-growth of the majority of images and toprovide fixed-sized aperture ... aperture has a radius of rcore.26 Aperture flux 427 Error in

8 Feb 2007: Table 1. R Z Y J H Ks FROM. Time & depth on sky in coadded Tiles Depth (Vega) required 21.9 21.4 20.3 Science. ... Priorities of different areas? PI. Single Tile Strategy Parameters set. 3 Detector Integration Time (DIT) sec 20 10 6 PI.

3 Jul 2007: The absolute fluxcalibration is accurate to 20%–30%. Pointing was checked onthe source 1034293. ... HD 92945. K1 22 20–150 271 70 >0.002 40 Chen et al.

18 Sep 2007: Basedon these analyses, Rhee et al. revised the fraction of nearby Astars with detected 60mm excess to 20%. ... typesystems) and young Sun-like stars (20 among 200 of the Gand K stars).

3 Sep 2007: 1.311 2001-06-07 21:30:20 24.07 J 0.93 1826.1 8.4 0.15 0.17 0.30 w_20010607_06526_2 CIRSI_NGC135A ... 1.311 2001-06-07 21:30:20 24.07 J 1.03 1960.3 8.9 0.18 0.14 0.25 w_20010607_06526_3 CIRSI_NGC135A

18 Jul 2007: While ALMA can detect the brightest knownclass II disks out to 20 kpc, we are not aware of any young(< 10 Myr) cluster within the Milky Way which has a ... For example, extrapo-lation of the exoplanet semi-major axis distribution to 20 AUsuggests that

26 Apr 2007: The dashed lineis for a path in a disc with Rt = 20 AU. ... The disc is initially trun-cated at Rt = 20 AU unless otherwise stated.

24 Apr 2007: 20 have planets• 18 have debris detected with IRAS• 1 has both• stars with planets are metal-rich (Fischer & Valenti 2005). • ... http://www.ast.cam.ac.uk/wyatt. 20. The planetesimal belt. Consider planetesimals orbiting the star at a distance r

5 Jun 2007: 0 19.4(20.3) 20.2(21.1) 20.7(21.6) 0.94 10.0. ... 8 20.2 30.2Ks 40 0.74 13.5 18.2 20.1 33.1.