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11 - 20 of 416 search results for KaKaoTalk:vb20 200 where 0 match all words and 416 match some words.

  1. Results that match 1 of 2 words

  2. VIRCAM Pipeline: vircam_matchxy.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__matchxy_8c-source.html
    10 Apr 2013: 00334 00335 cpl_msg_info(fctid,"Doing the matching for extension %d",j); 00336 (void)ps.cat1f), 00337 vircam_tfits_get_table(ps.cat2f),200.0, 00338 &(vircam_matchxy_config.xoff),

  3. VIRCAM Pipeline: vircam_tfits.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__tfits_8c-source.html
    10 Apr 2013: vircam_tfits.c. 00001 / $Id: vircam_tfits.c,v 1.13 2007/10/25 17:34:01 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

  4. VIRCAM Pipeline: vircam_utils.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__utils_8c-source.html
    10 Apr 2013: fitslist[i]); 01534 val = cpl_image_get_mean_window(im,100,100,200,200); 01535 if (val > lthr && val < hthr) 01536 fitslist[m++] = fitslist[i]; 01537 else 01538 if (ditch) 01539

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

    https://people.ast.cam.ac.uk/~wyatt/bkwj13.pdf
    14 Nov 2013: ity. 0. 6. 12. 18. 24. 30. 36. 20 200. 30.0Blackbody radius (AU).

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

    https://people.ast.cam.ac.uk/~wyatt/kw13.pdf
    16 Jul 2013: 88692 HD 165439 1.2 200 A2 11 Myr? Age uncertain? (22)89046 HD 166191 45.9? ... Inany case, removal of the coolest few sources (those below 200 Ksay) would make little difference to our analysis.

  7. arX iv:1 311. 2977 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf
    14 Nov 2013: Observations at wavelengths> 200 µm are sensitive to dust that is large enough totrace the planetesimal distribution.

  8. mnr_15360

    https://people.ast.cam.ac.uk/~wyatt/mw09.pdf
    17 Apr 2013: At this radius, the time-scale for planet stir-ring is only 0.65 Myr, orders of magnitude less than the star’s age(200 Myr; Barrado y Navascues et al.

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

    https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf
    29 Oct 2013: 2010). Possible (< 3σ) detection of orbital motionη Tel-B 48 2 200 6 Neuhäuser et al.

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

    https://people.ast.cam.ac.uk/~wyatt/vewt13.pdf
    8 Oct 2013: 10. 20. 50. 100. 200. Rkpc. UHk. msL. UHRL u sed fo r flyby co m pu tatio n s.

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

    https://people.ast.cam.ac.uk/~wyatt/vmbw13.pdf
    12 Apr 2013: 100 AU. 200 AU. 500 AU. 1000 AU. Figure 6. The number of orbits taken by an isolated planet arounda star throughout its MS phase.

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