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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. -
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. -
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. -
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. -
https://people.ast.cam.ac.uk/~rgm/wfcsur/int_ao.txt
https://people.ast.cam.ac.uk/~rgm/wfcsur/int_ao.txt1 Mar 1998: Name of PI and affiliation Names of CoIs with affiliation Postal and email address of PI Summary of proposal (max 200 words) List of targets with filter passbands & exposure times Page -
VIRCAM Pipeline: vircam_tfits.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__tfits_8c-source.html10 Apr 2013: vircam_tfits.c. 00001 / $Id: vircam_tfits.c,v 1.13 2007/10/25 17:34:01 jim Exp $ 00002 00003 This file is part of the VIRCAM Pipeline 00004 Copyright (C) 2005 Cambridge Astronomy Survey Unit 00005 00006 This program is free software; you can -
WFCAM simulations
https://people.ast.cam.ac.uk/~wfcam/docs/reports/simul/index.html3 Sep 2007: artdata. A full-well capacity of 200,000 electrons was used for the saturation level. -
Hard XMM sources
https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hr3-err_gt0.html27 Mar 2002: 0.853.08. A 1837. 200. 2001-02-22. Y. -1.7. -1.8. 20.7. 0. 22.6. ... 0.210.31. A 1837. 200. 2001-02-22. Y. -1.4. 1.4. 15.5. -1. 17.4. -
Graphics produced by IDL
https://people.ast.cam.ac.uk/~vasily/sdss/orphan/orphan6.pdf10 Apr 2009: 2. 3. 4. log(. g). 4.0 3.9 3.8 3.7 3.6log(Teff). 300 200 100 0 100 200 300Radial velocity (Galactic frame). ... 0. 20. 40. 60. Dec. 250 200 150 100RA. Orphan Stream: 17 < g < 19 => 20 < BHB distance (kpc) < 50.
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