Search
Search Funnelback University
31 -
40 of
365
search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk
where 0
match all words and 365
match some words.
Results that match 1 of 2 words
-
..............................................................…
https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf19 Apr 2006: This 200-AU-sized regioncoincides with the slightly tilted inner disk identified optically withthe Hubble Space Telescope5. ... The possible relationship of these components has yetto be explored, but the lower inferred temperatures of the clumpparticles -
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 -
Chapter 2 : Operating the software
https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter2.htm15 Nov 1998: Base Electronics base pixel value, typically 200-1000 and is updated periodically. -
Modeling the Structures of Dusty Disks: UnseenPlanets? Mark C. ...
https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf19 Apr 2006: 200 100 0 -100 -200RA offset, AU. -200. -100. 0. 100. ... 200. Dec. off. set,. AU. FIGURE 5. Impact of the outward migration of a Neptune mass planet on a planetesimal disk aroundVega [27]: orbital distribution of planetesimals at the beginning (top -
MNRAS 000, 1–11 (2020) Preprint 26November 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/zcac20.pdf26 Nov 2020: 8 A. Zurlo et al. 0 50 100 150 200 250 300Semi-major axis (au). ... Semi-major axis (au). 0. 50. 100. 150. 200. 250. Tota. l dus. -
Draft version July 18, 2022Typeset using LATEX default style ...
https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf22 Mar 2024: collisional evolution. Only 6 systems with ages in the range 50 to 200 Myr were detected. ... The typical FWHM beam size of 1.′′5 (200 au) comfortably encompasses dust belts with radii up to 100 au. -
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 -
Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …
https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf18 Apr 2022: 11 174718. 11910 123109310. 638406 245. Number of detectable planets. 0 200 400. ... Sub-Neptunes Sub-Jovians0. 50. 100. 150. 200. 250. 300. 350. Det. ecta.
Refine your results
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
Recent searches
Your search history is empty.