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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), -
Astroparticle_15
https://people.ast.cam.ac.uk/~gpe/Astroparticle_15.pdf25 Mar 2011: R is now 200 microns. This is very large on a quantum scale, but small on the scale used to test gravity in experiments – close to current limit of 100 -
arX iv:0 704. 0873 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf18 Apr 2007: 200. 7. Mon. Not. R. Astron. Soc. 000, 1–6 (2006) Printed 9 April 2007 (MN LATEX style file v2.2). ... Doppler systems arepredicted here to form from 5-200 Jupiter masses of gas inthe disk, enough to make gas giant planets. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf10 Nov 2017: Evidence for kinematically distinct outflows – discrete mass-loss episodes (strongly asymmetric)• Expansion velocities 40-50km/s• Kinematic age estimates for features, from distance/velocity, are 200, 400 and 900 years• Smallest -
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 -
Chapter 2 - Operating the software
https://people.ast.cam.ac.uk/~optics/cirsi/docs/pixcel/20010508/chapter2.htm16 Jun 2015: Base Electronics base pixel value, typically 200-1000 and is updated periodically. -
MNRAS 000, 1–6 (2016) Preprint 13 July 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/agwk16.pdf13 Jul 2016: 0 100 200 300 400 500. UV Distance [kλ]. 100. 0. ... 100. 200. 300. Re(v. ) [m. Jy]. 0 100 200 300 400. -
LOCAL HEATING IN THE GALACTIC CENTER WESTERN ARC N. ...
https://people.ast.cam.ac.uk/~wyatt/mtpf03.pdf19 Apr 2006: Dust emissionpeaks are resolved with source sizes of 200 to 500 (1.7 104 to4.3 104 AU). -
Debris discs around nearby solar analogues
https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf8 Jul 2009: e. upto approximately 200 au radius for stars at 12–15 pc distance. ... For five precise (G2 V) solar analogues,the fitted disc radii are 100–200 au (Krivov et al. -
L141 The Astrophysical Journal, 532:L141–L144, 2000 April 1q 2000. ...
https://people.ast.cam.ac.uk/~wyatt/ftpk00.pdf19 Apr 2006: Compared to the fullextent of the mid-IR–emitting size of the disk (200 AU), therelatively small values of the dust FWHM sizes suggest thatthe mid-IR emission is sharply peaked ... extends out to at least a radius of 100 (200 AU) fromthe star in the
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