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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. -
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 -
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 -
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. -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130626.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_130626.txt1 Jul 2013: The storage for the raw data for VST has also been reorganised using the new raid array on apm45. ... The good news is we passed with minor action items and ESO also agreed with our revised timetable for deliverables. -
Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf29 Oct 2013: r′t=t = a. (cos(f0 f)sin(f0 f). ) µai. (cos(nit)sin(nit). )(6). in the new astrocentric frame, where f =GM/a3t.
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