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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.

  1. Results that match 1 of 2 words

  2. ..............................................................…

    https://people.ast.cam.ac.uk/~wyatt/tfwd05.pdf
    19 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

  3. VIRCAM Pipeline: vircam_matchxy.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__matchxy_8c-source.html
    10 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),

  4. Astroparticle_15

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_15.pdf
    25 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

  5. Chapter 2 : Operating the software

    https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter2.htm
    15 Nov 1998: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  6. Modeling the Structures of Dusty Disks: UnseenPlanets? Mark C. ...

    https://people.ast.cam.ac.uk/~wyatt/wyat04a.pdf
    19 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

  7. MNRAS 000, 1–11 (2020) Preprint 26November 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/zcac20.pdf
    26 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.

  8. Draft version July 18, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 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.

  9. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf
    10 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

  10. VIRCAM Pipeline: vircam_utils.c Source File

    https://people.ast.cam.ac.uk/~wfcam/docs/vista/vircam_manual/vircam__utils_8c-source.html
    10 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

  11. Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …

    https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf
    18 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.

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