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5 Jun 2007: 7. Legacy value, serendipity, curiosity and new classes of object, 21st century Infra-Red equivalent of thePalomar-UK-ESO Schmidt Surveys. ... ESO Public Surveys Proposal Form Phase 1. 2. To discover objects cooler than the T-dwarfs and define the new Y

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.

1 Feb 2008: This is still ongoing research but isleading to new perspective on debris disk evolution. ... New Hub-ble/ACS observations in scattered light show that the inner“warp” in β Pic is really a secondary disk inclined by 5with respect to the primary disk.

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

17 Dec 2008: Greater planetary masses during the migratory stagecould allow the planets to self-excite to much greater eccentricities.Therefore, we run a new suite of simulations to look at the effectof

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.

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

15 Sep 2009: or more planets. Combining this new data with 42 already published observa-.

19 Jun 2009: Mon. Not. R. Astron. Soc. 000, 000–000 (2009) Printed 19 June 2009 (MN LATEX style file v2.2). The History of the Solar System’s Debris Disc: ObservableProperties of the Kuiper Belt. Mark Booth1?, Mark C. Wyatt1, Alessandro Morbidelli2, Amaya

4 Apr 2011: 1. SETTING THE SCENE. From the perspective of astronomers, the first decade of the new millennium has been termed the era ofprecision cosmology, when the parameters that describe our Universe have –

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

8 Jul 2008: For a parent with an orbit defined by a ande broken up at a true anomaly f , the new orbital elements are.

23 Mar 2007: 2005)(e.g., Fig. 1), the main new result of Su et al. ... used the new distributions of 24 and 70 µm excesses asa function of age shown in Fig.

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

5 Jul 2011: Wealso present new SPIRE images of the disc at 250 µm, as well as new constraints on the discfrom SCUBA-2, mid-IR and scattered light imaging. ... Stock et al. (2010) present new 10 µm nulling interferometrydata from the Keck Interferometer Nuller (KIN)

5 Oct 2007: Spitzer. IRS observations of the Deep Impact experiment in July 2005 created a new paradigm for under-. ... new species was allowed, and only species that reduced the χ2ν below the 95% confidence limit.

29 Apr 2008: In3 the various observational and analysistechniques employed for each instrument are outlined, and insection4 a new method of placing quantifiable extension lim-its on unresolved disk images is described. ... 4.1. A new method of determining extension

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

16 Nov 2021: a new solution for a star of a different totalmass M ′ simply by multiplying the other physical variables by appropriatescaling factors.

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.