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VIRCAM Pipeline: vircam_photcal.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__photcal_8c-source.html10 Apr 2013: cpl_table_and_selected_float(stds,junk,CPL_LESS_THAN,0.1); 00243 } 00244 00245 / Now extract all those that have passed the test. ... cpl_table_and_selected_float(stds,junk,CPL_LESS_THAN,0.1); 00658 } 00659 00660 / Now extract all those that have passed -
mnr_15360
https://people.ast.cam.ac.uk/~wyatt/mw09.pdf17 Apr 2013: We shall consider only secular perturbations. In the following,unsubscripted orbital elements refer to test particles and subscriptedto the planet(s). ... The Laplace–Lagrange theory describes well the behaviourof test particles, except for those near -
25The Messenger 147 – March 2012 Gerry Gilmore1,* Sofia ...
https://people.ast.cam.ac.uk/~gil/Gaia-ESO-Mess.pdf9 Oct 2013: Thus, these models require calibration with well-studied (nearby) test cases. For example, star formation involves turbulence, magnetic reconnec-tion, collisionless shocks, and radiative transfer through a turbulent medium. ... in the Plane to test -
VIRCAM Pipeline: vircam_linearity_analyse.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__linearity__analyse_8c-source.html10 Apr 2013: mjd,cdata,cf,fac; 00481 double facrng,maxdiff,lindata; 00482 vir_fits darks,domes,outfits,test,outdark,fframe; 00483 parquet pp; 00484 cpl_parameter p; 00485 cpl_propertylist drs,plist; 00486 ... fits_get_image(test)); 00667 vircam_fits_delete(test); -
MNRAS 433, 2334–2356 (2013) doi:10.1093/mnras/stt900Advance Access…
https://people.ast.cam.ac.uk/~wyatt/kw13.pdf16 Jul 2013: MNRAS 433, 2334–2356 (2013) doi:10.1093/mnras/stt900Advance Access publication 2013 June 12. The bright end of the exo-Zodi luminosity function: disc evolutionand implications for exo-Earth detectability. G. M. Kennedy‹ and M. C. WyattInstitute -
MNRAS 435, 1037–1046 (2013) doi:10.1093/mnras/stt1293Advance Access…
https://people.ast.cam.ac.uk/~wyatt/phwk13.pdf12 Nov 2013: Of all ourtargets, only HD 115617 (61 Vir) exhibits a large proper motion of(1070.36, 1063.69) mas yr1, enabling such a test within a rea-sonable time-span, as -
Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf29 Oct 2013: Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed 29 October 2013 (MN LaTEX style file v2.2). Imaged sub-stellar companions: not as eccentric as theyappear? The effect of an unseen inner mass on derivedorbits. Tim D. Pearce?, Mark C. Wyatt and -
STARS draft version, October 28, 2012 2 Contents 1 ...
https://people.ast.cam.ac.uk/~stars/doc/stars.pdf14 Mar 2013: STARS. draft version, October 28, 2012. 2. Contents. 1 Introduction 51.1 About the code. 51.2 About this document. 6. 1.2.1 Motivation. 61.2.2 Structure. 61.2.3 Further work. 6. 2 Basic user guide 92.1 Files. 92.2 Running the code. 92.3 Viewing -
arX iv:1 302. 3615 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/vmbw13.pdf12 Apr 2013: arX. iv:1. 302. 3615. v1 [. astr. o-ph. EP]. 14. Feb. 2013. Mon. Not. R. Astron. Soc. 000, 1–24 (2013) Printed 18 February 2013 (MN LATEX style file v2.2). Simulations of two-planet systems through all phases of stellar. evolution: implications
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