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15 Dec 2003: Telescope work on V2 packages 2 2 4. 4Casu. New Hire recruitment delays Hired JMI Personnel temporary hire 3 1 3. ... Personnel 4 week contingency 4 2 8. 6Casu. Software problems in development of new algorithms Software be smarter 2 2 4.

18 Jul 2003: 020 1.3 days before new moon, RA and dec: 7 21 50, 25 19.2 The sun is down for 10.1 hr; 7.4 hr from eve->morn 18

15 Aug 2003: He is in touch with Bertin to further this. JRL asked about the parameter order in the new catalogue software. ... There has been no further news about the new job contracts.

18 Jul 2003: 111 3.3 days before new moon, RA and dec: 5 32 26, 24 47.8 The sun is down for 10.1 hr; 7.4 hr from eve->morn 18

19 Jun 2003: Future equipment needs were discussed. STH and JRL need new new desktops. ... of JRL and STH PSB Organise rack mounting of JRL's SUN equipment for move to APM building MJI New actions ------------ STH finish setting up photometric standard fields MJI

18 Jul 2003: 057 2.3 days before new moon, RA and dec: 6 26 28, 25 42.8 The sun is down for 10.1 hr; 7.4 hr from eve->morn 18

31 Aug 2003: He is awaiting a reply. [Received following reply shortly after the meeting included here for ease of reference] "No, no new data - we've had problems with the detectors - damage due ... simulations, image subtraction and DQC] New Actions ----------- ALL

23 Jan 2003: with some tuning during commissioning and science verification. Further products ---------------- PSF generation methods, oversampled spatially varying PSFs good news, how to form them cf.

18 Jul 2003: The ESO Sky Calendar Tool. See alsoAlmanac. Roque de los Muchachos, La Palma. Tue, July 22, 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: Tue, 2003 Jul

12 Sep 2003: Preparation for camera design review meeting 7. AOB: (in)visibility of CASU web pages on new IoA web site Minutes ------- 1. ... Comments on WFAU minutes No new minutes were available since the previous CASU meeting, so there were no comments.

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.