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Planetary System DynamicsPart III Mathematics / Part III Astrophysics …
https://people.ast.cam.ac.uk/~wyatt/psd_eg1.pdf29 Sep 2023: e) Derive an expression for the distance of the particle P from the geometric centre of the ellipse O, andhence show that to first order in eccentricity the distance OP is -
Microsoft PowerPoint - Project_1640_optics
https://people.ast.cam.ac.uk/~optics/project1640/Project_1640_optics.pdf16 Jun 2015: Op. tic. al. de. sig. n c. an. be. bro. ke. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture05.pdf13 Oct 2014: The full calculation of stellar opacities is a major endeavour. For this rea-son, the Opacity Project (op) was set-up in 1984 as an international collab-oration to calculate the ... Similar work conducted at the LawrenceLivermore National Laboratory, the -
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https://people.ast.cam.ac.uk/~wyatt/wyat03a.pdf19 Apr 2006: "!# $&% ' )(# -,/.0-%12 &!$3542,67,98/:<;=?> @A>BDCFEGIHJ8K>L>MONPEQRCFSUTV8WX>YZ>L[GIEE]E[_7=?>Ya>bCFcXdGIHe_UNPEgfMhC[cA:QUeiPGkjEmlPG#QU_UmSn;opQqGI_U_#8rMhC[cX:Qq]iPG$st8vuFwPwPx>yopzV>|{-}8vuP{}Ic>yopQU]#GpPwgfT2C[Qqi:NPdEiV9bKhw{Pu&}&}P<As>. -
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduct…
https://people.ast.cam.ac.uk/~optics/cirsi/ociw/lco1999may/eric/reduction_manual16 Jun 2015: Look at the '.cl' files in home$wfirc/scripts for details. avgo n1 n2 chip op! ... imexam' cursor. To scale the skies to each other! use op = y dall n1 loop! -
Noname manuscript No.(will be inserted by the editor) Space-based ...
https://people.ast.cam.ac.uk/~wyatt/dlab18.pdf31 Jul 2018: JPL Publication. Lawson PR, Lay OP, Johnston KJ, Beichman CA (2007) Terrestrial PlanetFinder Interferometer Science Working Group Report. ... NASA STI/ReconTechnical Report N 8. Lay OP (2004) Systematic Errors in Nulling Interferometers. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture02.pdf10 Oct 2023: Magnitudes andluminosities are normally measured through a given filter; Figures 2.4 and2.5 show the transmission curves of some of the most commonly used op-tical and near-infrared filters. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi.guide.html16 Jun 2015: 2 FILTER7=Hn FILTER6=Jn FILTER5=Hl FILTER4=Hx FILTER3=Hs FILTER2=Jg FILTER1=Op FILTER0=Dk 13) Contact info, phone numbers, etc LCO during day this number is routed to -
Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…
https://people.ast.cam.ac.uk/~wyatt/swd08.pdf29 Apr 2008: We con-sider a detection to be whereS op > 3. 4.1.1. ... Ndθ = 0.1(dθ/θ)1010(r/θ)R0.5λ Ftot. with Nop andS op determined from equation 1. -
Observing guide for CIRSI (WFIRC) at LCO du Pont ...
https://people.ast.cam.ac.uk/~optics/cirsi/cirsi-guide-lco-0.6.html16 Jun 2015: 2 FILTER7=Hn FILTER6=Jn FILTER5=Hl FILTER4=Hx FILTER3=Hs FILTER2=Jg FILTER1=Op FILTER0=Dk 13) Contact info, phone numbers, etc LCO during day this number is routed to -
Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…
https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf22 Mar 2024: For the clustering of data and to guide the interpretation, wealso extracted environmental data from either the adaptive op-tics telemetry3 or the Astronomical Site Monitor (ASM) of theCerro Paranal Observatory4. ... We found much lower correlation rates -
arX iv:1 709. 0841 4v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/mcka17.pdf26 Sep 2017: three disks. For HD 131488, even the 13CO line is op-. ... tically thick with an optical depth of 5.7, while for. HD 121191 and HD 121617 this line was found to be op-tically thin. -
ms.dvi
https://people.ast.cam.ac.uk/~wyatt/wmke16.pdf10 Nov 2016: With the advent of an extreme adaptive op-tics instrument like the Spectro-Polarimetric High-contrastExoplanet REsearch (SPHERE; Beuzit et al. -
Draft version December 23, 2016Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cmws17.pdf23 Dec 2016: It summarizes previous findings aswell as results from this work. EC acknowledges support from NASA through HubbleFellowship grant HST-HF2-51355 awarded by STScI, op-erated by AURA, Inc. -
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https://people.ast.cam.ac.uk/~wyatt/wdt00.pdf19 Apr 2006: "! $#&%(')! ,.-/%103246587797: 0<;=>&?%/3#60A@ B4%)CD0CEGFHI6KJ&0ML80ONPRQ8%S 4T0. UWVYXOZ [MV6]AXV_ba c&dfehgjiZ k.l<]m.XOV$c=nPo$Zpp.V6qUhal VC]rsZ qoftuvxw=y"z. {}|x|C) 9(A6Wf69O6AR.E&RAAA9E9 //.¡¢E£¤E(¥ª«¢¥ª<E4OP/GK=. |Y|&µEºA)»|&{f| -
arX iv:1 702. 0512 3v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/bfwv17.pdf5 May 2017: The calculations sofar have focused on the geometrical optical depth of the op-tically thin dust, τ. ... edge. Such dust, how-ever, would produce a detectable infrared excess, as for op-tically thin discs, there is insufficient gas released for -
A planet-forming circumbinary disc in a polar configura-tion Grant ...
https://people.ast.cam.ac.uk/~wyatt/kmfm19.pdf17 Jan 2019: We can estimate a minimum CO mass by assuming that the CO emission is marginally op-. -
ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf19 Apr 2006: ApJ accepted, 7 November 2005Preprint typeset using LATEX style emulateapj v. 04/21/05. DUST IN RESONANT EXTRASOLAR KUIPER BELTS — GRAIN SIZE AND WAVELENGTH DEPENDENCEOF DISK STRUCTURE. M. C. Wyatt1. UK Astronomy Technology Centre, Royal -
arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf27 Jan 2016: 2014; Veillet et al. 2014). The LBT is locatedon Mount Graham in southeastern Arizona and is op-erated by an international collaboration among institu-tions in the United States, Italy, and ... The op-tics provide a field of view of 1010 arcsec2 with -
arX iv:1 201. 1911 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kwsd12.pdf12 Jan 2012: 2004), an adaptive op-tics image taken using the Lick Observatory Shane 3m tele-scope with the IRCAL near-IR camera as an ongoing search forfaint companions of stars in the ... To try and resolve this issue we obtained an adaptive op-tics image of 99 Her
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