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8 Mar 2006: GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad band background. ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of 0.1 per cent are needed compared with 1%

15 Apr 2006: Infrared OH Sky Observations: Mahaira etal, 1993, PASP. GOOD NEWS. The 1.0 to 1.8 micron IR sky is very dark between the OH lines which contain 95% of broad ... THE NOT SO GOOD NEWS. The narrowest gaps are narrower than in the optical; filter widths of

5 Oct 2006: If yes, explain why the need for new data. Are the data requested in this proposal on the ESO Archive (http://archive.eso.org)?

6 Jun 2006: 1. Legacy value, serendipity, curiosity and new classes of object, 21st century Infra-Red equivalent of thePalomar-UK-ESO Schmidt Surveys. ... 2. To discover objects cooler than the T-dwarfs and define the new ‘Y’ spectral class.

9 Oct 2006: This required a total time of 7359hrs based on VISTA ETC(v1.1).With the new VISTA ETC(v1.3) this reduces to a total of 6750hrs. ... PSP Panel Issue 5 The Panel strongly recommends that the PI submits a new proposal whichfocused on the science that can be

18 Jul 2006: The Panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in JK only.

18 Jul 2006: The Panel strongly recommends that the PI submits a new proposal which focused on the science that can be achieved by covering the whole southern sky in JK only.

17 Mar 2006: o Legacy value, Serendipity and new classes of object. o Maximising the science return from ESA missions, XMM-Newton, Planck, Herschel and GAIA.

9 Jan 2006: RGM noted that this was an impressive achievement to start the New Year with. ... UKIRT There is no new data for the UKIRT archive at the moment.

2 Feb 2006: DWE said that this would be sorted out with the new Plone system. ... ETC - This new CASU requirement occupied most of PSB's (& some of MJI's) time during January.