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https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/wfc_bynight.txt
https://people.ast.cam.ac.uk/~xmmssc/xid-imaging/wfc_bynight.txt19 Feb 2003: data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.080/0.004/0.016/17:a href=./lplogs/20000725.int:: ... Y:Y /data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.095/0.005/0.022/18:a href=./lplogs/20000726.int:: -
https://people.ast.cam.ac.uk/~xmmssc/xidops/xmmssc_optobs/pcms_summary…
https://people.ast.cam.ac.uk/~xmmssc/xidops/xmmssc_optobs/pcms_summary_20011120.comm10 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? -
Mark Wyatt
https://people.ast.cam.ac.uk/~wyatt/15 Apr 2024: Mark Wyatt. My research mostly focusses on the formation and evolution of stars and their planetary systems. In particular I am interested in the dusty debris material that surrounds some stars, including the Sun, during their main sequence phase. -
https://people.ast.cam.ac.uk/~xmmssc/xid/wfc_bynight.txt
https://people.ast.cam.ac.uk/~xmmssc/xid/wfc_bynight.txt17 Nov 2005: 3:PATT-XID:Y:Y /data/cass36h/wfc_nonsurvey/watson_jul2000_reduced/:Y:Y:Y:S:S:S:S:0.080/0.004/0.016/17:./lplogs/20000725.int:: ... 26:3:PATT-XID:Y:Y -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p2.pdf5 Jun 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J. -
ESO Survey Management Plan Form:VISTA Hemisphere Survey Phase 1 ...
https://people.ast.cam.ac.uk/~rgm/vhs/smp/SMP_VHS_v1p1.pdf23 Nov 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J. -
arX iv:1 310. 6936 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/gkte13.pdf28 Oct 2013: von Braun K. et al., 2011, ApJ 729, L26. Watson C.A. -
arX iv:1 408. 4116 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kw14.pdf22 Aug 2014: arX. iv:1. 408. 4116. v1 [. astr. o-ph. EP. ] 18. Aug. 201. 4Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 20 August 2014 (MN LATEX style file v2.2). Do Two Temperature Debris Disks Have Multiple Belts? G. M. Kennedy, M. C. WyattInstitute -
arX iv:1 309. 1466 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwbw13.pdf23 Jul 2014: primordial protoplanetary disk (Watson et al. -
ApJ409619o.dvi
https://people.ast.cam.ac.uk/~wyatt/lwcm11.pdf23 Feb 2012: was performed, with 1 cycle of 6 s integration at eachposition (Watson et al. -
arX iv:1 311. 2977 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf14 Nov 2013: 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. -
Five steps in the evolution from protoplanetary to debrisdisk ...
https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf17 Dec 2014: Five steps in the evolution from protoplanetary to debrisdisk. M. C. Wyatt • O. Panić • G. M. Kennedy •. L. Matrà. Abstract The protoplanetary disks seen around Her-big Ae stars eventually dissipate leaving just a tenuousdebris disk, -
TLA_large
https://people.ast.cam.ac.uk/~wyatt/tgmk14.pdf4 Dec 2014: MNRAS 445, 2558–2573 (2014) doi:10.1093/mnras/stu1864. An unbiased study of debris discs around A-type stars with Herschel. N. D. Thureau,1‹ J. S. Greaves,1 B. C. Matthews,2,3 G. Kennedy,4 N. Phillips,5. M. Booth,2,3,6 G. Duchêne,7,8 J. -
arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf29 Apr 2016: arX. iv:1. 604. 0828. 6v1. [ast. ro-p. h.E. P]. 28 A. pr 2. 016. DRAF T VERS IONA P RIL 29, 2016Preprint typeset using LATEX style emulateapj v. 5/2/11. POLARIZATION MEASUREMENTS OF HOT DUST STARSAND THE LOCAL INTERSTELLAR MEDIUM. J. P. MARSHALL 1,2, -
Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...
https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf2 Nov 2015: Accepted to ApJ: October 28, 2015Preprint typeset using LATEX style emulateapj v. 5/2/11. YOUNG “DIPPER” STARS IN UPPER SCO AND ρ OPH OBSERVED BY K2. M. Ansdell1,10, E. Gaidos2,3,4,10, S. A. Rappaport5, T. L. Jacobs6, D. M. LaCourse6, K. J. Jek6 -
, DRAFT VERSION DECEMBER 23, 2017Typeset using LATEX twocolumn ...
https://people.ast.cam.ac.uk/~wyatt/baaa18.pdf23 Dec 2017: WATSON,130 R.C. WEIR,4. KLAUS WENZEL,131 MICHAEL W. WILLIAMSON,56 JASON T. WRIGHT,10, 11, 132 M. -
Space Science Reviews manuscript No.(will be inserted by the ...
https://people.ast.cam.ac.uk/~wyatt/wj16.pdf15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant -
Analysis of the Herschel DEBRIS Sun-like star sample
https://people.ast.cam.ac.uk/~wyatt/skwl18.pdf19 Feb 2018: MNRAS 475, 3046–3064 (2018) doi:10.1093/mnras/stx3188Advance Access publication 2017 December 11. Analysis of the Herschel DEBRIS Sun-like star sample. B. Sibthorpe,1,2‹ G. M. Kennedy,3 M. C. Wyatt,4 J.-F. Lestrade,5 J. S. Greaves,6. B. C. -
MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mcwb18.pdf31 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. -
arX iv:1 511. 0591 9v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dmkw15.pdf25 Nov 2015: arX. iv:1. 511. 0591. 9v1. [ast. ro-p. h.E. P]. 18 N. ov 2. 015. Mon. Not. R. Astron. Soc.000, 1–18 (2002) Printed 19 November 2015 (MN LATEX style file v2.2). IR-excesses around nearby Lambda Boo stars are caused by debrisdisks rather than ISM
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