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2 Jul 2010: last bits of calibration plan document update RGM still testing and noted a 1% difference at the 5-sigma level between the different ways people are estimating the magnitude error due

30 Apr 2007: Yes otherwise = chaos. This is the usual precedent and will encourage people who have signed up to turn up.

5 Mar 2014: 11. AOB ------- On Tuesday the South African Science Minister and his entourage of 20+ people dropped by as part of an almost surprise visit during a tour of the new Battcock

16 Dec 2008: MJI noted that various people including Google Sky and MicroSoft are interested in IPHAS mosaics of the Galactic Plane.

24 Mar 2010: EGS will make it so. 8. AOB MJI gave a summary of the news about the various grants that CASU people are involved in this round and those that have been

17 Mar 2004: A number of people asked what exactly do we deliver to ESO?

26 Oct 2010: It will have a halon gas fire extinguishing system which means people will have to enter the building through the dog flap in pairs for 'elf & safety.

16 Jun 2015: Click the thumbnail for a full size picture. Andrew Dean <ajd@ast.cam.ac.uk>. page generated by web_thumbnail.pl V1.2. Last modified: Fri Aug 9 23:21:05 BST 2002.

6 Mar 2003: Ok but if we opt for WCS dependent info in columns we should use doubles for RA Dec in case people use them for other purposes.] 4.3 Other data product

9 Jan 2006: The status of this request is still unclear. RGM reported that most of the problems arose from people using the wrong parameters or not tuning the matching criteria appropriately.

4 Nov 2013: Part of the reason we made the cataloguing code available was for people to do exactly these sort of tests.

22 Oct 2011: Various people, VVV in particular, want to do catalogue completeness tests - excellent!

23 Sep 2013: An upcoming HAWK-I special calibration request to observe the same globular cluster in each of the four detectors in order to derive the relative zeropoint offsets suggests people are having

4 Sep 2012: Bo Milvang-Jensen demonstrated that people do actually use the CASU VISTA QC tables by asking for them to be updated.

16 Jun 2015: Picture gallery. David King <king@ast.cam.ac.uk>. Last modified: Fri Feb 21.

16 Jun 2015: J. =22.6 in an exposure time of only 90 minutes. So why are most people sceptical about using fibres for ultra-faint spectroscopy?

16 Jun 2015: the idea is to have only one copy on disk of data read from tape, in some default location like /data/cirsi/19991023, even if multiple people are running multiple pipelines

3 Nov 2000: 17 Aug 2000 run People working on CIRSI and helping with problems at some point during the run: Mark Phillips (mmp@lco.cl) Eric Persson (epersson@ociw.edu) Christoph Birk