Search

3 Dec 2010: 7. VISTA Update --------------- A new disk arrived, even as we met, containing data up to and including the 13th October. ... Horizon's are a bugger. 9. AOB -------- The new VISTA storage space system - a Supermicro - apparently is sentient, i.e.

1 Mar 2010: already in the SM and the new ones. b) For the new gauge bosons (not in the standard model), write down their charge, colour.

30 Aug 2010: To cut a long story short, this turned out to be due to a new and little used sky estimation option (simplesky - only used for the SV NGC253 project v1.0). ... Following JRL's lead a new policy was converged upon. If the data is good enough to process

5 May 2010: First are MJI's Fortran versions which are generally used as standalone applications and which MJI also uses to prototype new ideas. ... We all wish him well in his new enterprise and noted with amusement that he will once again be Paul Hirst's boss.

24 Mar 2010: Neither JAC nor CASU have budgetted for this since the requirement is a new one. ... Monthly progress and summary reports completed. 13th September - new version of ESO WFCAM FITS header document.

5 Oct 2010: def@subeqnnum{{reset@fontrm (thesubequation)}} % % A new label command to refer to subequations.

27 May 2010: All three stars are known disc hosts.Herschel spatially resolves the dust emissionaround all three stars (marginally, in the case ofβ UMa), providing new information about discs as close as 11

2 Sep 2010: The de-bris absorbs starlight and re-emits it at longer wavelengths,and observations since 2003 with the Spitzer space telescopehave yielded many new debris detections in the mid- to ... 3 OBSERVATIONS AND DATA REDUCTION. The eleven new stars were

10 Nov 2010: 5. Discussion and conclusions. Using new mid-IR images at 18 and 25µm, we have confirmedthe previously observed brightness asymmetry discovered byTelesco et al. ... 350,Hipparcos, the New Reduction of the Raw Data. Wahhaj, Z., Koerner, D.

22 Aug 2010: arX. iv:1. 008. 0865. v2 [. astr. o-ph. SR. ] 6. Aug. 201. 0. Mon. Not. R. Astron. Soc.000, 1–11 (2010) Printed August 9, 2010 (MN LATEX style file v2.2). Resolved Imaging of the HD191089 Debris Disc. Laura Churcher1, Mark Wyatt1, Rachel

27 Jul 2010: Parameter Orginal value New value. Mmid 10.0 7.8 MDc 60.0 1.9kme 0.05 0.05. ... lation that incorporates the optical properties of realisticgrains, to find new values for this parameter set.

6 Apr 2010: Su et al. (2006) presented new 24 and 70µmphotometry which also confirms the excess.

15 Dec 2010: arX. iv:1. 012. 3079. v1 [. astr. o-ph. EP. ] 14. Dec. 201. 0. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 15 December 2010 (MN LATEX style file v2.2). A general model of resonance capture in planetary systems:First and second order

25 Nov 2010: arX. iv:1. 011. 4858. v1 [. astr. o-ph. EP]. 22. Nov. 201. 0Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 November 2010 (MN LATEX style file v2.2). Collisional Evolution of Irregular Satellite Swarms:. Detectable Dust around Solar

19 Feb 2010: When stirring reachesthe outer edge, all disks break to a faster decline in fbecause no new regions can be stirred.