Search

Search Funnelback University

Search powered by Funnelback
10 results 20 results 50 results
Relevance Date (Newest first) Date (Oldest first) Title (A-Z) Title (Z-A) Distance URL (A-Z) URL (Z-A) Shuffle
31 - 40 of 46 search results for KaKaoTalk:PC53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 46 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. VIRCAM Pipeline: vircam_dark_combine.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__dark__combine_8c-source.html
    10 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

  4. 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).

  5. 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.

  6. 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.

  7. 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.

  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. 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.

  10. 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

  11. 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

Refine your results

clear all

Date

Search history

Recently clicked results

Recently clicked results

Your click history is empty.

Recent searches

Recent searches

Your search history is empty.