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VIRCAM Pipeline: vircam_dark_combine.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__dark__combine_8c-source.html10 Apr 2013: 00329 return(-1); 00330 00331 / Create the parameters list in the cpl_recipe object / 00332 00333 recipe->parameters = cpl_parameterlist_new(); 00334 00335 / Fill in the parameters. ... First the combination type / 00336 00337 p = cpl_parameter_new_range( -
VIRCAM Pipeline: vircam_jitter_microstep_process.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__jitter__microstep__process_8c-source.html10 Apr 2013: 00269 recipe->parameters = cpl_parameterlist_new(); 00270 00271 / Fill in the minimum object size / 00272 00273 p = cpl_parameter_new_value("vircam.vircam_jitter_microstep_process.ipix", 00274 CPL_TYPE_INT, ... documentation fix 01035 01036 Revision 1.12 -
VIRCAM Pipeline: vircam_dome_flat_combine.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__dome__flat__combine_8c-source.html10 Apr 2013: new(); 00335 00336 / Lower threshold for rejecting underexposed images / 00337 00338 p = cpl_parameter_new_value("vircam.vircam_dome_flat_combine.lthr", 00339 CPL_TYPE_DOUBLE, 00340 "Low rejection threshold for ... 01345 01346 Revision 1.1 2006/02/27 -
MNRAS 435, 1037–1046 (2013) doi:10.1093/mnras/stt1293Advance Access…
https://people.ast.cam.ac.uk/~wyatt/phwk13.pdf12 Nov 2013: time. One, or possibly two, of these new detections islikely a background source. ... New, high-sensitivity detections area path towards investigating the trends in dust mass evolution. -
VIRCAM Pipeline: vircam_twilight_flat_combine.c Source File
https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__twilight__flat__combine_8c-source.html10 Apr 2013: recipe object / 00343 00344 recipe->parameters = cpl_parameterlist_new(); 00345 00346 / Lower threshold for rejecting underexposed images / 00347 00348 p = cpl_parameter_new_value("vircam.vircam_twilight_flat_combine.lthr", 00349 ... 44:47 jim 01430 new -
STARS draft version, October 28, 2012 2 Contents 1 ...
https://people.ast.cam.ac.uk/~stars/doc/stars.pdf14 Mar 2013: Thisis sometimes useful when creating new models. 1. IX Determines whether hydrogen is converted into helium. ... Setting this to 5 will usethe new opacity tables with variable C/O composition. -
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: parameters list in the cpl_recipe object / 00345 00346 recipe->parameters = cpl_parameterlist_new(); 00347 00348 / Fill in the parameters. ... mean(ps.lchantab,"lin_10000_err"); 01178 01179 / Save new linearity info / 01180 01181 if -
arX iv:1 311. 2947 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bkwj13.pdf14 Nov 2013: By studying debris discs orbit-. 1 exoplanet.eu. ing these ‘retired’ A stars, we access a new popu-lation of planetary systems, from which more canbe learnt regarding the structure and ... As further detections of debris discs orbitingsubgiants are -
arX iv:1 302. 7000 v2 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bkcj13.pdf12 Apr 2013: Acceleration dvdt. 1.51 0.52ms1yr1. Table 1. The new best-fit orbital parameters for κ CrB b derivedfrom the continued radial velocity monitoring at the Lick andKeck observatories. ... Figure 1. Radial velocity monitoring of κ CrB over -
mnr_15360
https://people.ast.cam.ac.uk/~wyatt/mw09.pdf17 Apr 2013: With this in mind, we define a new parameter which describesthe boundary between planet-stirred and self-stirred regions of the.
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