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  2. 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
  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_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.
  5. 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),
  6. 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.
  7. 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.
  8. 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.
  9. 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.
  10. 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
  11. 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!

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