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31 - 40 of 45 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 45 match some words.

  1. Results that match 1 of 2 words

  2. VIRCAM Pipeline: vircam_detector_noise.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__detector__noise_8c-source.html
    10 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

  3. arX iv:1 311. 2947 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/bkwj13.pdf
    14 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).

  4. MNRAS 435, 1037–1046 (2013) doi:10.1093/mnras/stt1293Advance Access…

    https://people.ast.cam.ac.uk/~wyatt/phwk13.pdf
    12 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.

  5. mnr_15360

    https://people.ast.cam.ac.uk/~wyatt/mw09.pdf
    17 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.

  6. arX iv:1 302. 7000 v2 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/bkcj13.pdf
    12 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.

  7. arX iv:1 302. 3615 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/vmbw13.pdf
    12 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.

  8. VIRCAM Pipeline: vircam_jmp_utils.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__jmp__utils_8c-source.html
    10 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

  9. VIRCAM Pipeline: vircam_reset_combine.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__reset__combine_8c-source.html
    10 Apr 2013: 01149 Revision 1.24 2006/05/16 13:58:47 jim 01150 Fixed memory leaks that occur from not closing images at the end of 01151 the image extension loop 01152

  10. STARS draft version, October 28, 2012 2 Contents 1 ...

    https://people.ast.cam.ac.uk/~stars/doc/stars.pdf
    14 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

  11. 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.

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