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13 Mar 2012: VHS Survey Management Wiki (some pages are public). News. Proposal. ... Proposal Planning Wiki [hosted on Astrogrid Wiki]. Brief description of baseline survey [v3] [out of date; new version in preparation].

22 May 2012: Another new instrument with sensitivity to hot dust is the Palomar Fiber Nuller (PFN; Hanot et al.2011). ... A new generation of coronagraphs behind extreme AO systems on 8-meter-class ground-based tele-scopes is in the development and commissioning phase

9 Oct 2012: 2.3 New Accretion Rate Calculations. Assuming 0.01 solar composition by mass, extrapolated fromcalcium abundance, for both DAZ and DBZ white dwarfs isnot ideal, but understandable based on existing data ... 2.1 Steady State Metal Accretion. 2.2

12 Jan 2012: arX. iv:1. 201. 1911. v1 [. astr. o-ph. EP. ] 9. Jan. 2012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 11 January 2012 (MN LATEX style file v2.2). 99 Herculis: Host to a Circumbinary Polar-ring Debris Disk. G. M. Kennedy1, M. C. Wyatt1,

1 Aug 2012: New for this work was theadditional requirement of including a separate population oflarge cool grains with a > 100 μm. ... preferentially vaporizing the small end of an initial dust pop-ulation, leaving behind a remnant large dust population and

5 Oct 2012: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 3 October 2012 (MN LATEX style file v2.2). Resolved Debris Discs Around A Stars in the HerschelDEBRIS Survey? Mark Booth1,2†, Grant Kennedy3, Bruce Sibthorpe4, Brenda C. Matthews2,1,Mark C.

24 Feb 2012: In prep. ABSTRACT. We present new MIDI interferometric and VISIR spectroscopic observations ofHD113766 and HD172555.

7 Jul 2012: 2009; Bryden et al. 2009;Dodson-Robinson et al. 2011). However, there is new tentative ev-idence that nearby stars with low-mass planetary systems are morelikely to harbour debris than

7 Nov 2012: Physics, University of New South Wales, Sydney 2052, Australia15Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA.

19 Jun 2012: The semi-major axis, eccentricity and inclinationof the new orbits of the debris (a′, e′, I′) will be given by:.

19 Jan 2012: pronounced atλ 70µm.Here we present new simulations that show that this connection is qualitatively robust to a range of parameters: the massdistributionof the giant planets, the width and mass distribution

23 Feb 2012: Itis important to note, however, that while our spectral modelingtechniques can provide important new information, they are alsocomplex. ... A number of new mineralspecies were studied and compared to the η Corvi spectrum,in an attempt to match the