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MNRAS 435, 1037–1046 (2013) doi:10.1093/mnras/stt1293Advance Access…
https://people.ast.cam.ac.uk/~wyatt/phwk13.pdf12 Nov 2013: Ithas been verified against high-S/N 24 µm MIPS photometry for tar-gets within the Herschel open time key project Disc Emission via a. ... 2005) was imaged at 24 and 70 µm using Spitzer(Su et al. -
25The Messenger 147 – March 2012 Gerry Gilmore1,* Sofia ...
https://people.ast.cam.ac.uk/~gil/Gaia-ESO-Mess.pdf9 Oct 2013: Korn 19, ‡. Alessandro Lanzafame 20, ‡. Elena Pancino 17, ‡. Ernst Paunzen 21, ‡. Alejandra Recio-Blanco 22, ‡. Giuseppe Sacco 2, ‡. Rodolfo Smiljanic 23, ‡. Sophie Van Eck 24, ‡. Nicholas Walton 1, ‡. 1 Institute of ... Barcelona; 24 -
VIRCAM Pipeline: vircam_wcsutils.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__wcsutils_8c-source.html10 Apr 2013: Modified to use cpl_wcs interface 00786 00787 Revision 1.25 2007/10/25 17:34:01 jim 00788 Modified to remove lint warnings 00789 00790 Revision 1.24 ... 1.11 2006/06/13 14:09:54 jim 00831 Added vircam_removewcs 00832 00833 Revision 1.10 2006/05/24 -
Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf29 Oct 2013: 2012)HR 8799-b 39 1 68 2 Marois et al. (2008). -c - 38.0 1.0 --d - 24.5 0.6 --e - 14.6 0.4 Marois et al. -
VIRCAM Pipeline: vircam_matchstds.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__matchstds_8c-source.html10 Apr 2013: 00500 Revision 1.2 2006/04/27 14:22:05 jim 00501 Fixed docs 00502 00503 Revision 1.1 2006/04/24 10:42:45 jim 00504 New routine 00505 00506 -
arX iv:1 311. 2947 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bkwj13.pdf14 Nov 2013: 75 2.61 1.0 0.1HD 1502 1342225479/10 2011-07-24 12.4 1.61 4915 159.2 2.4 0.5 1.64 0.03 0.65 ... ity. 0. 6. 12. 18. 24. 30. 36. 20 200. 30.0Blackbody radius (AU). -
arX iv:1 302. 7000 v2 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bkcj13.pdf12 Apr 2013: Accepted 2013 February 24. Received 2013 February 22; in original form 2012 December 20. ... Spitzer 24 766 13 800.1 0.1 8.0a. Spitzer 70 83 2 426.2b 6.5 22.3a. -
VIRCAM Pipeline: vircam_genlincur.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__genlincur_8c-source.html10 Apr 2013: 00001 / $Id: vircam_genlincur.c,v 1.24 2008/01/22 19:45:24 jim Exp $ 00002 00003 This file is part of the VIRCAM Pipeline 00004 Copyright (C) 2005 ... Place, Suite 330, Boston, MA 02111-1307 USA 00019 / 00020 00021 / 00022 $Author: jim $ 00023 $Date: 2008 -
arX iv:1 302. 3615 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/vmbw13.pdf12 Apr 2013: c 2013 RAS, MNRAS 000, 1–24. Full-Lifetime Two-Planet Simulations 5. These trends are model-dependent. ... A reduction of the star’s mass by a factor. c 2013 RAS, MNRAS 000, 1–24. -
mnr_15360
https://people.ast.cam.ac.uk/~wyatt/mw09.pdf17 Apr 2013: Whether thisis sufficient to stir a disc depends on the typical size of bodies in thedisc (see equations 23 and 24). ... 2007), removed. Ofthese 57 stars, 10 show significant excess emission at 24 μm and/or70 μm, and are classed as disc hosts.
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