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1 - 10 of 40 search results for `good news` |u:people.ast.cam.ac.uk

  1. Fully-matching results

  2. 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

  3. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 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

  4. CASU analysis of SV data for WFCAM

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/sv/index.html
    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

  5. Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...

    https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf
    12 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.

  6. https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/summary…

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/commissioning/summary.txt
    4 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

  7. Quasars and Galaxies at the Highest Redshifts

    https://people.ast.cam.ac.uk/~rgm/presentations/20050922-Crafoord-Symposium.ppt
    8 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%

  8. Data Processing Philoshpy

    https://people.ast.cam.ac.uk/~wfcam/docs/philosophy01.html
    23 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,

  9. Oxford Meeting

    https://people.ast.cam.ac.uk/~rgm/presentations/20060412-SKA-Meeting_Oxford.ppt
    15 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

  10. Data Processing Philoshpy - 23rd January changes highlighted

    https://people.ast.cam.ac.uk/~wfcam/docs/philosophy02.html
    19 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

  11. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_111123.txt
    19 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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