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41 - 46 of 46 search results for katalk:za33 24 |u:people.ast.cam.ac.uk where 0 match all words and 46 match some words.

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  2. MNRAS 433, 2334–2356 (2013) doi:10.1093/mnras/stt900Advance Access…

    https://people.ast.cam.ac.uk/~wyatt/kw13.pdf
    16 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.

  3. VIRCAM Pipeline: vircam_twilight_flat_combine.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__twilight__flat__combine_8c-source.html
    10 Apr 2013: 12:40 jim 01352 Removed calls to vircam_ndit_correct as this is now no longer necessary 01353 01354 Revision 1.24 2007/02/06 13:11:12 jim 01355 Fixed ... update 01369 01370 Revision 1.19 2006/11/10 09:24:49 jim 01371 Fixed bug in save routine where the

  4. VIRCAM Pipeline: vircam_dome_flat_combine.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__dome__flat__combine_8c-source.html
    10 Apr 2013: Also fixed memory deallocation error in tidy routine 01269 01270 Revision 1.25 2006/09/29 11:19:31 jim 01271 changed aliases on parameter names 01272 01273 Revision 1.24

  5. Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf
    29 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.

  6. VIRCAM Pipeline: vircam_linearity_analyse.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__linearity__analyse_8c-source.html
    10 Apr 2013: vircam_linearity_analyse.c. 00001 / $Id: vircam_linearity_analyse.c,v 1.51 2008/01/22 19:47:56 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

  7. arX iv:1 310. 1395 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vewt13.pdf
    8 Oct 2013: Υxy|max =2GMr3Hill,x. (23). and. |Υxx|max = |Υyy|max =GMr3Hill,x. G2. (24). Having defined the Hill ellipsoid and related it to the mag-nitude of the perturbations, we can

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