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15 Apr 2024: Hull C. L. H., Yang H., Cortes P. C., Dent W. ... Cotton D. V., Marshall J. P., Frisch P. C., Kedziora-Chudzer L., Bailey J., Bott K., Wright D.

12 Oct 2021: H. Chen, A. Morlok, D. M. Watson, P. Manoj, P. Sheehan, T. ... Page, P. Panuzzo, A. Papageorgiou, C. P. Pearson, I. Perez Fournon,M.

22 May 2012: H. Chen, T. P. Greene, P. M. Hinz, M. J.Kuchner, C. ... H., Sheehan, P., Watson, D. M., Manoj, P., & Najita, J.

11 Apr 2019: Cotton1,2?, Jonathan P. Marshall3,4, Priscilla C. Frisch5,Lucyna Kedziora-Chudzer1,2, Jeremy Bailey1,2, Kimberly Bott6,7,Duncan J. ... 2010;Cotton et al. 2016b,c; Frisch et al. 2016; Cotton et al.

8 Jan 2019: Matrà7. and M. C. Wyatt11Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK2Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany3Astrophysikalisches Institut und Universitätssternwarte

6 Apr 2010: Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. ... Smith and M.C. Wyatt: Warm dusty discs: Exploring the A star 24µm debris population 3.

25 Oct 2009: c 0000 RAS, MNRAS 000, 000–000. 4 M. C. Wyatt et al. ... c 0000 RAS, MNRAS 000, 000–000. 6 M. C. Wyatt et al.

7 Jul 2012: c 0000 RAS. 2 G. M. Kennedy, M. C. Wyatt. 1984; Kalas et al. ... 5 Retrieved fromhttp://skyview.gsfc.nasa.gov/. c 0000 RAS, MNRAS000, 000–000.

21 Jan 2014: 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al. ... 100. 50. 0. 50Z. [p. c]. 200 150 100 50 0 50Y [pc].

18 Aug 2020: as. tro-. ph.E. P] 1. 7 A. ug 2. 020. 2 Krivov and Wyatt. ... star (1 <p<2), we mayexpect that larger discs tend to be more massive.

29 Apr 2008: as negative;b=Age taken from Geneva-Copenhagen Survey;c= Identified as having excess by Hines. ... 2. Dec. offs. et, a. rcse. c. Residuals. 2 1 0 -1 -2RA offset, arcsec.

10 Feb 2021: 2020TheAuthors. arX. iv:2. 010. 1265. 7v1. [as. tro-. ph.E. P] 2. ... Significant emission is notedwith eitheran "A", "B" or "C", and numerically counted ifmore than one source type in a single image is detected.

28 Oct 2013: et al., 2013, A&A 555, A11Eiroa C. et al., 2010, A&A 518, L131Figueira P. ... von Braun K. et al., 2011, ApJ 729, L26. Watson C.A.

22 Aug 2014: C. WyattInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK. ... component. c 0000 RAS, MNRAS000, 000–000. Two Temperature Debris Disks: Multiple Belts?

4 Dec 2014: 3 P R O P E R T I E S O F A - S TA R D E B R I S D I S C S. ... 0P. 160. R16. 0χ. 160. nam. ety. pe(p. arse. c)(M. yr).

29 Apr 2016: Filter HD T/C λeff q u p d p/d θ[nm] [ppm] [ppm] [ppm] [pc] [ppm/pc] []. g′ 2262 Target 464.2 4.7 5.7 37.4 ... Sub-micron (0.1µm) dust grains are predicted to have. 10 J. P.

14 Nov 2013: of Fomalhaut b, though itnow appears to apply to a hypothetical Fomalhaut c(Chiang et al. ... 2009).The suggestion that the entire HR 8799 system may be. coplanar is consistent with the results of Watson et al.(2011) and Greaves et al.

17 Dec 2014: Five steps in the evolution from protoplanetary to debrisdisk. M. C. ... M. C. Wyatt. O. Panić. G. M. Kennedy. L. Matrà. Institute of Astronomy, University of Cambridge, MadingleyRoad, Cambridge CB3 0HA, UK.

19 Feb 2018: 3 D I S C I N C I D E N C E A R O U N D F, G , A N D KT Y P E S TA ... 4(c), is 28 per cent,the same as that given in Table 2.

31 Jul 2018: S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S. Casassus4,5, V. ... P] 3. Jul. 201. 8. 2 S. Marino et al. than 10 au it has only been possible to detect a few gas gi-ants, mainly through direct imaging 1 (Marois

25 Nov 2015: Z. H. Draper1,2, B. C. Matthews2,1, G. M. Kennedy3, M. C. ... Continued. c 2002 RAS, MNRAS000, 1–18. 6 Z. H. Draper et al.

2 Jul 2014: Jonathan P. Marshall1,2,, A. Moro-Martı́n3,4, C. Eiroa1, G. Kennedy5, A. Mora6, B. ... J.P. Marshall, A. Moro-Martı́n, et al.: Herschel observations of exoplanet host stars.

7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. ... scattered disks. M. C. Wyatt1, A. Bonsor1, A. P. Jackson2, S.