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  2. Cambridge STARS Homepage

    https://people.ast.cam.ac.uk/~stars/
    28 Feb 2013: In most circumstances, just 200 points are sufficient. Simultaneous solution of structure and composition.
  3. STARS draft version, October 28, 2012 2 Contents 1 ...

    https://people.ast.cam.ac.uk/~stars/doc/stars.pdf
    14 Mar 2013: Eachset of reaction rates comes as a block of 200 numbers in 20 rows and 10 columns, just like the charged particlereaction data.
  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt
    29 Mar 2013: For the record these are: 20121013 runs 200-205; 20121025 runs 130-139; 20121112 runs 155-168 = not exactly a massive haul!
  5. 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
  6. VIRCAM Pipeline: vircam_tfits

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/group__vircam__tfits.html
    10 Apr 2013: Returns:. The output vircam_tfits object list. Author:. Jim Lewis, CASU. Definition at line 200 of file vircam_tfits.c.
  7. 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),
  8. 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
  9. 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.
  10. 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.
  11. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt
    28 May 2013: For the record, previous (re)processed nights were for missing Chilean data 20121013 200-205 20121025 130-139 20121112 155-168 ] We also spotted since the beginning of P91 that ESO

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