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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. -
VIRCAM Pipeline: vircam_tfits.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__tfits_8c-source.html10 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 -
VIRCAM Pipeline: vircam_tfits
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/group__vircam__tfits.html10 Apr 2013: Returns:. The output vircam_tfits object list. Author:. Jim Lewis, CASU. Definition at line 200 of file vircam_tfits.c. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130227.txt29 Mar 2013: For the record these are: 20121013 runs 200-205; 20121025 runs 130-139; 20121112 runs 155-168 = not exactly a massive haul! -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130431.txt28 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 -
VIRCAM Pipeline: vircam_matchxy.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__matchxy_8c-source.html10 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), -
VIRCAM Pipeline: vircam_utils.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__utils_8c-source.html10 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 -
Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf29 Oct 2013: 2010). Possible (< 3σ) detection of orbital motionη Tel-B 48 2 200 6 Neuhäuser et al. -
arX iv:1 311. 2947 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bkwj13.pdf14 Nov 2013: ity. 0. 6. 12. 18. 24. 30. 36. 20 200. 30.0Blackbody radius (AU). -
arX iv:1 311. 2977 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf14 Nov 2013: Observations at wavelengths> 200 µm are sensitive to dust that is large enough totrace the planetesimal distribution.
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