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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

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,

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.

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

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

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

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:

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

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).

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.