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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

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

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

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.

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%

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,

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

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

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

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

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

12 Mar 2009: He also noted the hardware server moves to the new room over last w/e and wondered if the ensuing silence was good news or bad news. ... The other piece of good news is that this mod can be back-propagated to all the earlier catalogues from 05A -, i.e.

27 Apr 2012: No news is still good news from the point of view of the next installment of ESO Phase 3 deliverables. ... A celebratory glass, or two, of fizz was imbibed to celebrate JRL's good news.

10 Feb 2012: Apparently SCUBA-2 is working well on JCMT which is good news for continuing access to UKIRT, and the Korean interest in WFCAM time is extending to include another Institution. ... No news is probably good news from the point of view of the next

11 Mar 2011: Henry from UltraVISTA and found that though the artifacts around bright stars have gone away, acquiring an example of their deep stack image to investigate other issues would be good news - ... WFCAM update ---------------- The weather at UKIRT has

28 Aug 2012: Just goes to prove that getting our VISTA calibration paper(s) out as soon as possible is good news. ... Video board changes usually imply gain changes implying further still that a comparison of pre- and post-board change flats would be good news.

17 May 2005: This is very good news since the full non-linearity correction is computationally intensive (currently 30s per pawprint). ... There was a discussion on what observations were needed for regularly generating good master flats.

5 Dec 2012: The good news is these two effects cancel out such that the ensuing derived magnitudes are correct, the bad news is that we are going to fix them all anyway. ... 10. ESO in-kind stuff --------------------- Nothing to report this month other than the good

3 Jan 2008: VISTA news - pipeline progress - camera test data - VISTA QC and operations - ESO SMP letters to PIs 8. ... 7. VISTA news VISTA: WJS reports that the primary mirror now has a good fringe pattern right out to the edges, meaning that the extent of the

2 Jul 2010: He also noted that the calibration units have been installed and after a few flux level tests good linearity sequences et al. ... can still access them remotely as needed SC - does our ZFS need a good tune?