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17 Oct 2013: Professor Efstathiou has received several prizes for his research including the 1990 Maxwell Medal and Prize of the Institute of Physics, the 1990 Vainu Bappu Prize of the Astronomical Society of

16 Jun 2015: [Local pages. Telescope projects. Observatories/Departments. There is a comprehensive list of observatories maintained by the RGO. ESO On-Line Information System. Instrumentation Groups. Detectors. Software Applications/Packages. FITS. URL http://www

24 Jul 2019: Nov. 90. Dark energy and the ever-expanding Universe. Maxwell Society lecture, King's London.

22 Oct 2017: Reaction Rate for Fusion. We have the velocity in terms of the particle energies already and the distribution of particle energies is given by the Maxwell-Boltzmann distribution:. ... Substitute expression for cross-section into equation for the

9 Oct 2017: Atoms, mass m, in thermal equilibrium in stellar atmosphere. • Random motion obeying Maxwell-Boltzmann distribution, most probable speed vmp =(2kT/m)1/2. • ... Velocity, v, from the Maxwell-Boltzmann distribution, vmp = (2kT/m)1/2 , and. •

21 Feb 2011: p e H γ. Assume that the particle densities are given by the non-relativistic Maxwell-Boltzmann formula.

23 Oct 2023: We obtain this by recalling that thedistribution of particle velocities as a function of T is given by the Maxwell-Boltzmann distribution:. ... With the Maxwell-Boltzmann distribution in energy terms:. nE dE =2n. π1/21.

15 Apr 2024: The optical constants for these grains are added together assuming various ratios for the components using Maxwell-Garnett effective medium theory.

27 Feb 2012: No evidence seen so far - still agree with Maxwell! But monopoles arise naturally in GUTs and other theories based on large gauge groups!

19 Apr 2006: Our 850 mm map, obtained with the Submillimeter Common-UserBolometric Array on the James Clerk Maxwell Telescope, shows three peaks of emission at the 2.5 mJy levelin the vicinity of

17 Nov 2020: the lowest momentum state, in accord with the 1-D Maxwell-Boltzmanndistribution:. P(px) dpx =(. 1. 2π mkT. )1/2exp.  p2x2mkT.  dpx (12.9)shown on the right side ... The normal Maxwell-Boltzmann distribution of protonenergies serves to define

19 Apr 2006: 1999) wasused on the James Clerk Maxwell Telescope (JCMT) toobtain deep simultaneous images of Fomalhaut at wave-lengths of 450 and 850 lm.

6 Nov 2018: In statistical equilibrium at temperature T,the number density nx of particles with mass mx is given by the Maxwell-Boltzmann equation:.

19 Apr 2006: 1999) at the James Clerk Maxwell Telescope wasused to observe τ Ceti in 2001 September and November, for a totalintegration time of 13.3 h.

8 Jul 2009: 2 S U RV E Y D ATA. The SCUBA camera on the 15 m James Clerk Maxwell Telescope(JCMT) was used to survey G-dwarf (luminosity class V or

19 Apr 2006: 2 OBSERVATIONS. Sub-mm observations were made using the SCUBA bolome-ter array on the James Clerk Maxwell Telescope. ... Details of Maxwell-Garneteffective medium theory, and the methods used to calculateabsorption efficiencies are discussed in Bohren &

13 Oct 2014: 3.4);. 4. The kinetic temperature, defined by the Maxwell-Botzmann distribu-tion:. nv dv = n.

18 Sep 2007: ABSTRACT. We present the scientific motivation and observing plan for an upcoming detection survey fordebris disks using the James Clerk Maxwell Telescope. ... SCUBA-2 (Holland et al. 2006) is a new submillimeter cam-era arriving at the James Clerk

21 Jul 2016: The James Clerk Maxwell Telescope is operated by the EastAsian Observatory on behalf of The National Astronomical Ob-servatory of Japan, Academia Sinica Institute of Astronomy andAstrophysics, the Korea Astronomy and

12 Oct 2021: Fitzgerald, Maxwell A. Millar-Blanchaer, GaspardDuchêne, Jennifer Patience, Justin Hom, Marshall D.

3 Jul 2007: SCUBA camera on the James Clerk Maxwell Telescope.

19 Apr 2006: 2. OBSERVATIONS. 2.1. Submillimeter. The submillimeter observations of Corvi were made usingthe Submillimeter Common-User Bolometer Array (SCUBA)at the James Clerk Maxwell Telescope (JCMT).

14 Mar 2013: It is based on A Simple Makefile Tutorial 1, whichWarrick Ball found on the website of Bruce Maxwell. ... 1http://www.cs.colby.edu/maxwell/courses/tutorials/maketutor/. 9. OPACITY OUT OF RANGE TF FR FKL FKH. followed by four numbers.

22 Mar 2024: Leisenring,19. Maxwell A. Millar-Blanchaer,20 Laurent Pueyo,7 Shrishmoy Ray ,17 Steph Sallum,21 Karl R.

12 Nov 2013: In the frame-work of the ongoing SCUBA-2 Observations of Nearby Stars, the instrument SCUBA-2 on theJames Clerk Maxwell Telescope was used to provide measurements of 450 and 850

17 Oct 2022: and the most probablespeed is v =. 2kT/m for a Maxwell-Botzmann distribution. In cooler stars, where pressure broadening is most important, collisionswith neutral hydrogen atoms are the main source of

22 Aug 2010: 1999) using Maxwell-Garnett effective mediumtheory. The optical properties of the grains were calculated usingMie theory, Rayleigh-Gans theory and Geometric Optics in the ap-propriate size regimes (Bohren & Huffman 1983).

3 Nov 2008: 1999).Dielectric constants were calculated using Maxwell-Garnett ef-fective medium theory and optical properties calculated usingMie theory, Rayleigh-Gans theory and Geometric Optics in theappropriate size regimes (Bohren & Huffman 1983).

14 Sep 2015: 103 M in silicate grains mixed withices (using the Maxwell-Garnett rule).

24 Jan 2012: College, Cambridge.1984 Senior Research Fellowship King’s College, Cambridge.1990 Maxwell Medal & Prize Institute of Physics.1990 Vainu Bappu Prize Astronomical Society of India.1991 Fairchild Distinguished Scholar California Institute

10 Dec 2012: 2005; Beichman et al. 2006; Brydenet al. 2009), the James Clerk Maxwell Telescope (Hollandet al.

19 Apr 2006: The 850 µm map of Vega obtained by Holland et al.(1998) with the Submillimeter Common-User Bolome-ter Array (SCUBA) on the James Clerk Maxwell Tele-scope shows an extended,

27 Mar 2023: ar 2. 023. 2 M. Booth et al. Bolometer Array (SCUBA) image of the disc taken at theJames Clerk Maxwell Telescope (JCMT) (Greaves et al.1998), there have been claims of

19 Apr 2006: 1.Recently the structure of the disc was mapped at both 450 and850 µm using SCUBA at the James Clerk Maxwell Telescope(JCMT) (Holland et al. ... We usethe optical constants for each of the components taken from Li &Greenberg (1997, 1998) and compute

5 May 2017: 1991). With the introduc-tion of the Submillimetre Common-User Bolometer Array(SCUBA) to the James Clerk Maxwell Telescope (JCMT),Greaves et al.

5 May 2017: 2 (SCUBA2) installedin the James Clerk Maxwell Telescope (JCMT), thus, incorporatinginformation from small and large angular scale structure.

19 Apr 2006: RESONANT TRAPPING OF PLANETESIMALS BY PLANET MIGRATION: DEBRIS DISK CLUMPSAND VEGA’S SIMILARITY TO THE SOLAR SYSTEM. M. C. WyattUK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, UK; wyatt@roe.ac.uk. Received 2003 June 11;

24 May 2022: Sasha Hinkley ,1 Aarynn L. Carter ,2 Shrishmoy Ray ,1 Andrew Skemer,2 Beth Biller,3 Elodie Choquet,4 Maxwell A.

5 Jul 2011: 1999) using Maxwell-Garnetteffective medium theory. The optical properties of the grains werecalculated using Mie theory, Rayleigh-Gans theory and GeometricOptics in the appropriate size regimes (Bohren & Huffman 1983).This composition

16 Jun 2015: Recently,a dust halo was also detected in far-IR resolvedHerschelandJCMT (James Clerk Maxwell Telescope) images by Matthews etal.

22 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

10 Feb 2014: 2.2. Ground-based sub-millimeter observations. η Crv was observed as part of the SONS survey on the James Clerk Maxwell Telescope (JCMT).

19 Nov 2009: The Herschel space observatory and the SCUBA-2 camera on the JamesClerk Maxwell Telescope will allow efficient photometric surveying at 70 to 850 µm,which allow for the detection of cooler ... 2003; Audley et al. 2004) camera on theJames Clerk Maxwell