Search
Search Funnelback University
21 -
57 of
57
search results for watson |u:people.ast.cam.ac.uk
Fully-matching results
-
Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf29 Oct 2013: Le Bouquin et al. 2009; Watson et al.2011; Kennedy et al. -
arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf5 May 2017: arX. iv:1. 701. 0656. 8v1. [as. tro-. ph.S. R]. 23. Jan. 2017. rsos.royalsocietypublishing.org. Research. Article submitted to journal. Subject Areas:. astrophysics, extrasolar planets, stars. Keywords:. variable stars, protoplanetary disks,. debris -
arX iv:1 403. 6186 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mmek14.pdf2 Jul 2014: arX. iv:1. 403. 6186. v1 [. astr. o-ph. EP. ] 24. Mar. 201. 4Astronomy & Astrophysicsmanuscript no. dunes˙debris˙exoplanets˙v18 c ESO 2014March 26, 2014. Correlations between the stellar, planetary and debris componentsof exoplanet systems -
Observations, Modeling and Theory of Debris Disks Brenda C. ...
https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf7 Jan 2014: Observations, Modeling and Theory of Debris Disks. Brenda C. MatthewsNational Research Council of Canada – Herzberg Astronomy & Astrophysics. Alexander V. KrivovFriedrich-Schiller-Universität Jena. Mark C. WyattUniversity of Cambridge. Geoffrey -
arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot, -
https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt
https://people.ast.cam.ac.uk/~optics/cirpass/datared/list_xml.txt16 Jun 2015: Spot a 00:47:33.410 -25:17:13.6 Spot i 00:47:33.013 -25:17:18.12 Spot n 00:47:33.063 -25:17:17.20 -
Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...
https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf5 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. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090923.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090923.txt28 Sep 2009: MJI is in communication with Watson Varricatt regarding the low light level non-linearity tests and also a revisit of the normal non-linearity tests. ... Watson and MJI will also be comparing dome flats with twilight sky flats. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p1.pdf5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H. -
MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/kw20.pdf18 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 -
ESO Survey Management Plan Form:VISTA Hemisphere Survey Phase 1 ...
https://people.ast.cam.ac.uk/~rgm/vhs/smp/SMP_VHS_v0p501.pdf18 Feb 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J. -
MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwak20.pdf10 Feb 2021: MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled usingMNRASLATEXstyle file v3.0. ALMA Survey of Lupus Class III Stars: Early Planetesimal BeltFormation and Rapid Disk Dispersal. J. B. Lovell1,M.C.Wyatt1,M.Ansdell2,M.Kama3,1, G.M.Kennedy4,5, -
Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…
https://people.ast.cam.ac.uk/~wyatt/swd08.pdf29 Apr 2008: Astronomy & Astrophysicsmanuscript no. 8719 c ESO 2008April 28, 2008. The Nature of Mid-Infrared Excesses From Hot Dust AroundSun-like Stars. R. Smith1,2, M. C. Wyatt1, and W.R.F. Dent3. 1 Institute of Astronomy, University of Cambridge, Madingley -
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/ukirt0210/almanac.t…
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/ukirt0210/almanac.txt25 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 -
Publications of the Astronomical Society of Australia (PASA)doi:…
https://people.ast.cam.ac.uk/~wyatt/khna21.pdf23 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, -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_100630.txt2 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. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0_fjc.pdf5 Jun 2007: Viana(CAUP), F. Walter(MPIA), N. Walton(Cam), S. Warren(IC),M. Watson(Leic), N. Webb(Toulouse), J. -
arX iv:2 110. 0431 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wyat21.pdf12 Oct 2021: H. Chen, A. Morlok, D. M. Watson, P. Manoj, P. Sheehan, T. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_110126.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_110126.txt22 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. -
ms_v2.dvi
https://people.ast.cam.ac.uk/~wyatt/rcmw12.pdf22 May 2012: H., Sheehan, P., Watson, D. M., Manoj, P., & Najita, J. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120829.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120829.txt4 Sep 2012: Watson Varricat came up with an interesting problem relating to WFCAM and crowded field photometry, e.g. -
arX iv:1 008. 0865 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/cws10.pdf22 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 -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf24 Nov 2023: Watson, E. Westra, T. Wold & C. WolfNature 461, 1254-1257(29 October 2009)doi:10.1038/nature08459. -
842 Publications of the Astronomical Society of the Pacific, ...
https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf18 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 -
arX iv:s ubm it/03 5390 2 [ astr o-ph ...
https://people.ast.cam.ac.uk/~wyatt/bw11.pdf8 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 -
MNRAS 000, 1–12 (2018) Preprint 4 December 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/cmfk19.pdf11 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 -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/PS-VHS-v3p0.pdf6 Jun 2006: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H. -
Inner edges of planetesimal belts: collisionally eroded or truncated?
https://people.ast.cam.ac.uk/~wyatt/immb23.pdf20 Feb 2024: 2006 ), (14) Watson et al. ( 2011 ), (15) Sepulveda & Bowler ( 2022 ), (16) Mamajek & Bell ( 2014 ), (17) Plavchan et al. ( -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/wbpc09.pdf25 Oct 2009: Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 19 October 2009 (MN LATEX style file v2.2). Collisional evolution of eccentric planetesimal swarms. M. C. Wyatt1?, M. Booth1, M. J. Payne1, L. J. Churcher11 Institute of Astronomy, University -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: arX. iv:1. 002. 3469. v1 [. astr. o-ph. EP]. 18. Feb. 2010. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 19 February 2010 (MN LATEX style file v2.2). Are debris disks self-stirred? G. M. Kennedy and M. C. WyattInstitute of Astronomy, -
MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf8 Jan 2019: MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled using MNRAS LATEX style file v3.0. A gap in HD 92945’s broad planetesimal disc revealed byALMA. S. Marino1,2?, B. Yelverton1, M. Booth3, V. Faramaz4, G. M. Kennedy5,6, L. Matrà7. and M. -
hd113766_dust_25Sep2007
https://people.ast.cam.ac.uk/~wyatt/lcwm08.pdf5 Oct 2007: performed (Watson et al. 2004). The reduction and analysis of the spectra was conducted with. -
arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al. -
Observing Kepler stars with WISE
https://people.ast.cam.ac.uk/~wyatt/kw12.pdf7 Jul 2012: arX. iv:1. 207. 0521. v1 [. astr. o-ph. EP. ] 2. Jul 2. 012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 5 July 2012 (MN LATEX style file v2.2). Confusion limited surveys: using WISE to quantify the rarit y ofwarm dust around Kepler stars. -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: arX. iv:1. 004. 0644. v1 [. astr. o-ph. EP. ] 5. Apr. 201. 0Astronomy & Astrophysicsmanuscript no. astars˙3rd c ESO 2010April 6, 2010. Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. Wyatt2. 1 Astrophysics Group, -
The Astrophysical Journal, 701:2019–2032, 2009 August 20…
https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf1 Aug 2012: 2004). In order to avoid time-consuming peak-up, theobservatory was operated in IRS spectral mapping mode wherea 2 3 raster (spatial dispersion) centered on the star wasperformed (Watson et al.
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
- People aliens |u:www.enterprise.cam.ac.uk (2) · moments ago
Recent searches
Your search history is empty.