Search

5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

25 Sep 2002: ac.uk To: Weimin Yuan wmy@ast.cam.ac.uk, Jonathan Tedds jat@star.le.ac.uk, Mike Watson mgw@star.le.ac.uk Subject: Almanac Info for Dates of UKIRT

23 Nov 2021: Publications of the Astronomical Society of Australia (PASA)doi: 10.1017/pas.2021.xxx. The formation of planetary systems with SPICA. Kamp, I.1, Honda, M.2, Nomura, H.3, Audard, M.4, Fedele, D.5, Waters, L.B.F.M.6,7, Aikawa,Y.8, Banzatti, A.9, Bowey,

5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H.

18 Feb 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.

5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.

10 Feb 2002: e.q. 0100 0112570401 PROCESSING Dr Michael Watson M31 Core 00:42:43.0 41:15:46.0 59262 - - - - - - - - - - Flag of status: SAS ERROR (29) but PPS products exist?

12 Oct 2021: H. Chen, A. Morlok, D. M. Watson, P. Manoj, P. Sheehan, T.

5 Jun 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J.

31 Jul 2018: MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled using MNRAS LATEX style file v3.0. A gap in the planetesimal disc around HD 107146 andasymmetric warm dust emission revealed by ALMA. S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S.

18 Aug 2020: MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled using MNRAS LATEX style file v3.0. Solution to the debris disc mass problem:planetesimals are born small? Alexander V. Krivov1? and Mark C. Wyatt21Astrophysikalisches Institut und

2 Jul 2010: There has been a further shrinkage of staff at UKIRT. Tom Kerr is now our main contact with Watson the other UKIRT contact.

22 May 2012: H., Sheehan, P., Watson, D. M., Manoj, P., & Najita, J.

22 Feb 2011: Finally we note that Watson Varricatt took over from Chris Davis a few months ago as the official contact person for all matters relating to WFCAM data processing.

4 Sep 2012: Watson Varricat came up with an interesting problem relating to WFCAM and crowded field photometry, e.g.

24 Nov 2023: Watson, E. Westra, T. Wold & C. WolfNature 461, 1254-1257(29 October 2009)doi:10.1038/nature08459.

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

18 Sep 2007: 842. Publications of the Astronomical Society of the Pacific, 119: 842–854, 2007 August 2007. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A. An Unbiased Survey of 500 Nearby Stars for Debris Disks: A JCMT Legacy

8 Nov 2011: arX. iv:s. ubm. it/03. 5390. 2 [. astr. o-ph. EP]. 8 N. ov 2. 011. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 8 November 2011 (MN LATEX style file v2.2). The scattering of small bodies in planetary systems:. constraints on the possible

11 Apr 2019: MNRAS 000, 1–12 (2018) Preprint 4 December 2018 Compiled using MNRAS LATEX style file v3.0. The wavelength dependence of interstellar polarization inthe Local Hot Bubble. Daniel V. Cotton1,2?, Jonathan P. Marshall3,4, Priscilla C. Frisch5,Lucyna