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31 - 40 of 42 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 42 match some words.

  1. Results that match 1 of 2 words

  2. wyatt

    https://people.ast.cam.ac.uk/~wyatt/wyatt_lyot07.pdf
    18 Jun 2007: Late heavy bombardment model of (Gomes et al. 2005). 20. Conclusions 1 (Good news)Most disk radial structure explained by steady-state evolution of aplanetesimal belt due to collisions and radiation

  3. arX iv:0 704. 0873 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/gfwb07.pdf
    18 Apr 2007: 2005) findinga range from 72/1330 = 5.4 % within 5 AU up to an extrap-olation of 11 % within 20 AU. ... 2005, e.g) need a fewtimes the Minimum Mass Solar Nebula, which comprised ap-proximately 20 MJ up (Davis 2005).

  4. ESO Public Surveys Proposal Form Phase 1 Appendix B: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-Appendid-B-PSP-Response.pdf
    5 Jun 2007: Response: The original VHS proposal was a 7 year program which aimed to survey the full 20,000deg2 ofsouthern celestial hemisphere with exposure times of 180, 180, 60, 60 seconds in

  5. WFCAM Catalogues Document Number: VDF-SPE-IOA-00009-0001 Version 4…

    https://people.ast.cam.ac.uk/~rgm/vhs/smp/WFCAM-catalogues-v4p0.pdf
    19 May 2007: 20 Aperture flux 1 These are a series of different radii soft-edged apertures designed toadequately sample the curve-of-growth of the majority of images and toprovide fixed-sized aperture ... aperture has a radius of rcore.26 Aperture flux 427 Error in

  6. Guidelines_SMP_VISTA_03

    https://people.ast.cam.ac.uk/~rgm/vhs/smp/guidelinesVISTA_03.pdf
    8 Feb 2007: Table 1. R Z Y J H Ks FROM. Time & depth on sky in coadded Tiles Depth (Vega) required 21.9 21.4 20.3 Science. ... Priorities of different areas? PI. Single Tile Strategy Parameters set. 3 Detector Integration Time (DIT) sec 20 10 6 PI.

  7. MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...

    https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf
    3 Jul 2007: The absolute fluxcalibration is accurate to 20%–30%. Pointing was checked onthe source 1034293. ... HD 92945. K1 22 20–150 271 70 >0.002 40 Chen et al.

  8. 842 Publications of the Astronomical Society of the Pacific, ...

    https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf
    18 Sep 2007: Basedon these analyses, Rhee et al. revised the fraction of nearby Astars with detected 60mm excess to 20%. ... typesystems) and young Sun-like stars (20 among 200 of the Gand K stars).

  9. https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/summary.list

    https://people.ast.cam.ac.uk/~wfcam/docs/reports/dqc/raw/summary.list
    3 Sep 2007: 1.311 2001-06-07 21:30:20 24.07 J 0.93 1826.1 8.4 0.15 0.17 0.30 w_20010607_06526_2 CIRSI_NGC135A ... 1.311 2001-06-07 21:30:20 24.07 J 1.03 1960.3 8.9 0.18 0.14 0.25 w_20010607_06526_3 CIRSI_NGC135A

  10. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/wcg07.pdf
    18 Jul 2007: While ALMA can detect the brightest knownclass II disks out to 20 kpc, we are not aware of any young(< 10 Myr) cluster within the Milky Way which has a ... For example, extrapo-lation of the exoplanet semi-major axis distribution to 20 AUsuggests that

  11. arX iv:0 704. 3369 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/mlpw07.pdf
    26 Apr 2007: The dashed lineis for a path in a disc with Rt = 20 AU. ... The disc is initially trun-cated at Rt = 20 AU unless otherwise stated.

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