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search results for `good news` |u:people.ast.cam.ac.uk
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CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html26 Jan 2006: The good news is these artefacts are non-astronomical in appearance and do not "talk" across the detector quadrant boundaries, or between detectors; the bad news is that they do not ... of reset/reads, filter, persists over many frames etc. The good news -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060126.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060126.txt2 Feb 2006: MJI said in general that a small fraction of supposedly good frames were randomly selected and visually checked, though how many depended on which pipeliner. ... No news is good? news regarding the rest of the archives. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_060802.txt9 Aug 2006: 5. Data archives update AAT: No news is good news ING: JRL and EGS reported that the last 10 years of data (1996-2006) had now been ingested into Sybase. ... He will look into this. 7. WFCAM news Catalogue software: MR and EGS have been investigating the -
CASU analysis of SV data for WFCAM
https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/26 Jan 2006: The good news is these artefacts are non-astronomical in appearance and do not "talk" across the detector quadrant boundaries, or between detectors; the bad news is that they do not ... of reset/reads, filter, persists over many frames etc. The good news -
Quasars and Galaxies at the Highest Redshifts
https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt8 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% -
Oxford Meeting
https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt15 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
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