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MGB thesis Chapter 3
https://people.ast.cam.ac.uk/~optics/tech/mgb_phd/chapter3.htm16 Jun 2015: [Chapter 3: Camera. Outline. This chapter describes the near infrared camera built for COAST. It examines the properties required from the camera system, the range of devices available and the factors involved in the choice of detector. The design, -
L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...
https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the -
PDF/48/aa5873-06.pdf.url
https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf14 Dec 2006: 2004), we estimate for the firsttime the detection rate of cold debris disks around field M-dwarfs with ages between 20 and 200 Myr. ... al. 2005), the Castor moving group(200 Myr), the Ursa Maj moving group (500 100 Myr asrevised by King et al. -
Searching for Saturn's Irregular Satellite Swarm with Spitzer
https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf29 Jun 2012: Stansberry. OFF ON IE IW. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400. offs. et (. Sat. urn. radi. -
arX iv:a stro -ph/ 0504 086 v1 4 A ...
https://people.ast.cam.ac.uk/~wyatt/srms05.pdf19 Apr 2006: higher surface brightness at r >200 AU compared to the r4 power law. ... but has slightlyhigher surface brightness at r > 200 AU compared to ther4 power law. -
Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...
https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf21 Jul 2016: A 200 km/svelocity range is shown around the stellar velocity in the heliocen-tric frame of 23.0 0.3 km/s (Torres et al. ... The wide-fit baseline yields a 10.5 sigma detection of 200.0 19.1 mK km/s. -
Debris disk dynamical theory Mark Wyatt Institute of Astronomy, ...
https://people.ast.cam.ac.uk/~wyatt/MarkWyatt_Spitzer2008Conference.pdf12 Jan 2009: Radius, AU 200 400 600 800. Surf. ace. brig. htne. ss. -
MNRAS 000, 1–14 (2020) Preprint 8October 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/xkwy20.pdf8 Oct 2020: 2015).Assuming thepriors stated above,we ran LOFTI on the relative Gaia measurements until 200,000orbits were accepted, and plot the joint posterior distributions inFig. ... 160. 200. 240. []. 10 15 20. m [MJup]. m [MJup] = 1422. -
MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf22 Mar 2024: 200. 0. 200. 400. µJy. /Bea. m. Figure 1. Naturally weighted ALMA 880𝜇m images of our BPMG M-dwarf sample. ... 0. 200. 400. µJy. /Bea. m. Figure 2. Naturally weighted ALMA 880𝜇m image of TYC 7443-1102-1.The stellar location is marked with a. -
Draft version December 23, 2016Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cmws17.pdf23 Dec 2016: 100. 0. 100. 200. 300. 2.''. 118.AU. N. E. NICMOS, F110WALICE program. ... 2. 4. 1.10-6. 0.00001. 5.10-6. 200 100 0 100 200. 15.
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