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29 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

16 Jun 2015: Op. tic. al. de. sig. n c. an. be. bro. ke.

13 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

19 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>.

16 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!

31 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.

10 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.

16 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

29 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.

16 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

22 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

26 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.

10 Nov 2016: With the advent of an extreme adaptive op-tics instrument like the Spectro-Polarimetric High-contrastExoplanet REsearch (SPHERE; Beuzit et al.

23 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.

19 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|

5 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

17 Jan 2019: We can estimate a minimum CO mass by assuming that the CO emission is marginally op-.

19 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

27 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

12 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