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UKIDSS LAS intra-frameset inter-frame waveband positional offsets
https://people.ast.cam.ac.uk/~rgm/ukidss/framesets/8 Oct 2009: The good news is that the number of frames effected should not increase further(needs to be checked) so the fraction of pointings effected in this way should decrease in the -
wyatt
https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf18 Jun 2007: Good news for TPF (look at oldstars). Bad news for explaining systemswith 25µm excess many of whichhave f>1000fmax and so must betransient. ... Late heavy bombardment model of (Gomes et al. 2005). 20. Conclusions 1 (Good news)Most disk radial structure -
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 -
Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...
https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf12 Jan 2009: Sub-mm. Far-IR. Mid-IR. Good news: different wavelengths see different grain sizes and different structures. ... Bad news: both spatial distribution τ1/r and temperature of far-IR dust implies mass loss of 2M/Myr. -
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% -
Data Processing Philoshpy
https://people.ast.cam.ac.uk/~wfcam/docs/philosophy01.html23 Jan 2003: FWHM alternative: image FWHM summation out to kFWHM, since for standard profiles is at least as good as above two finely? ... with some tuning during commissioning and science verification. Further products ---------------- PSF generation methods, -
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 -
Data Processing Philoshpy - 23rd January changes highlighted
https://people.ast.cam.ac.uk/~wfcam/docs/philosophy02.html19 Mar 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. ... One of its conclusions was that nearest pixel gives very good -
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/summary…
https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/summary.txt4 Feb 2005: The good news is there are no measurable pixel-by-pixel differences within a channel. ... This is good news for offset restrictions within jitter sequences. The first pass astrometric residuals over the entire field are less than 100mas and the density -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt19 Dec 2011: then. The good news on the calibration front is that if we can solve the illumination correction problem, even with only the 3 SA's observed each night that form the ... The other good news is that the raw VST calibration and public survey data have all
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