Search

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%

19 Apr 2006: Here we present new mid-IR observations of the Vega-likestar HD 141569 (B9.5 Ve).

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 Apr 2006: A new 850-µmimage shows that there is indeed such a debris disc, extending out to 55 au (15 arcsec)radius.

16 Nov 2006: A set of components was tested. exhaustively before the addition of a new species was allowed, and only species that reduced. ... New work by Wyatt et al. (2007) also demonstrates that it is highly unlikely that an asteroid.

19 Apr 2006: 1999). Here we present new 10.8 and 18.2 km images, obtainedat the Keck II telescope, of the HR 4796A debris disk. ... Our new images clarify the structure of the central clear-ing zone, or hole, which may be indirect evidence for aplanet orbiting HR

19 Apr 2006: All rights reserved. Printed in U.S.A. et al. 2004). Since the three newly resolved disks are around Gand M stars, these new images are filling in our understanding ofhow ... TheIRAS fluxes were determined from SCANPI (IRAS Scan Pro-cessing and

19 Apr 2006: 2003). An informativeresult from the ISO survey (Habing et al. 2001) was that althoughthe sensitivity was five times greater than for the equivalent searchmade by IRAS, only one new disc was

19 Apr 2006: Table 1. New observations used in our analysis. Observationsbefore 2000 were extracted from the JCMT archive. ... The top part of the table shows new data, the bottom part showsexisting data.

6 Jun 2006: 1. Legacy value, serendipity, curiosity and new classes of object, 21st century Infra-Red equivalent of thePalomar-UK-ESO Schmidt Surveys. ... 2. To discover objects cooler than the T-dwarfs and define the new ‘Y’ spectral class.