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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 -
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. -
VIRCAM Pipeline: vircam_jitter_microstep_process.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__jitter__microstep__process_8c-source.html10 Apr 2013: few more changes to make sure that if things fail then it doesn't try 00996 and run further processing steps 00997 00998 Revision 1.24 2006/08/07 ... 24 jim 01011 Fixed a small memory leak and a bug in vircam_jmp_dither_offsets 01012 01013 Revision 1.19 -
VIRCAM Pipeline: vircam_dark_combine.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__dark__combine_8c-source.html10 Apr 2013: Revision 1.26 2006/04/25 13:45:56 jim 01326 Fixed to adhere to new calling sequence for vircam_dfs routines 01327 01328 Revision 1.25 2006/04/24 ... 46:35 jim 01329 A bit more error trapping in case fits structures can't be loaded 01330 01331 Revision -
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. -
MNRAS 433, 2334–2356 (2013) doi:10.1093/mnras/stt900Advance Access…
https://people.ast.cam.ac.uk/~wyatt/kw13.pdf16 Jul 2013: The W1 W3 distribution of the 24 174 stars is shown in Fig. ... There-fore, as with longer wavelengths (i.e. 24 µm; Siegler et al. -
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. -
STARS draft version, October 28, 2012 2 Contents 1 ...
https://people.ast.cam.ac.uk/~stars/doc/stars.pdf14 Mar 2013: r 26. Vhom9. m 18. L 27. U23 is the square of the radius of gyration; 24–26 are homology invariants. ... 23. 24. 4Code structure. A new section describing some of the broader things used in the code so that people know what they’re dealingwith when -
VIRCAM Pipeline: vircam_jmp_utils.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__jmp__utils_8c-source.html10 Apr 2013: vircam_jmp_utils.c. 00001 / $Id: vircam_jmp_utils.c,v 1.33 2008/07/10 13:05:53 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 -
VIRCAM Pipeline: vircam_detector_noise.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__detector__noise_8c-source.html10 Apr 2013: 49:39 jim 00874 Header comment update 00875 00876 Revision 1.24 2006/09/08 09:17:27 jim 00877 Modified to flag dummy results 00878 00879 Revision 1.23
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