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18 Jul 2003: The ESO Sky Calendar Tool. See alsoAlmanac. Roque de los Muchachos, La Palma. Wed, July 23, 2003. pseudo-Greenwich Daylight Savings Time assumed from 2 AM on 2003 Mar 30 to 2 AM on 2003 Sep 28; standard zone = 0 hrs W For the night of: Wed, 2003 Jul

18 Jul 2003: The ESO Sky Calendar Tool. See alsoAlmanac. Roque de los Muchachos, La Palma. Thu, July 24, 2003. pseudo-Greenwich Daylight Savings Time assumed from 2 AM on 2003 Mar 30 to 2 AM on 2003 Sep 28; standard zone = 0 hrs W For the night of: Thu, 2003 Jul

18 May 2003: DWE agreed with this. There is a new plan regarding the survey manager. ... MJI contact AA regarding new plan for survey manager (2 x 0.5 posts).

19 Mar 2003: Updated after detailed feedback from Steve Warren 23rd January 2003. Updated with new timescales 18th March. ... with some tuning during commissioning and science verification. Further products ---------------- PSF generation methods, oversampled

4 Jun 2003: MJI will discuss the new plan for a survey manager with AA at the Edinburgh meeting. ... MJI reported that the new CASU grant will be a revisable grant rather than a rolling grant.

1 Dec 2003: STH still needs to look at the spatial systematics in the UFTI standards (and new test) data MJI has not supplied WFAU with WFCAM-CIRSI test data with updated headers to ... FIRES comparisons STH look at the spatial systematics in the UFTI standards data

11 Dec 2003: If this is different from that in. modin. , the code should interpolate the given model to give the new one, provided that NCH is greater than or equal to 1.

16 Oct 2003: DWE placed interleaving report on public access side of web. ALL sent in summaries for our Q3 report and generated the new deliverables for Q4. ... New Actions ----------- MJI get more details about the QE variations of the 4 science-grade detectors MJI

5 Oct 2003: Simon Hodgkin, CASU. Funny Filters. YZ define new passbands. YZ can be bootstrapped into the Vega system.

20 Aug 2003: DETECTOR NOISE PROPERTIES. The detectors will be being used in a new mains power environment, attached to atelescope, and may have noise properties different to those measured in the lab.