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31 - 40 of 74 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 74 match some words.

  1. Results that match 1 of 2 words

  2. , EUROPEAN SOUTHERN OBSERVATORY Organisation Européenne pour des…

    https://people.ast.cam.ac.uk/~rgm/vhs/eso-p79b-vhs.pdf
    5 Oct 2006: whole southern celestial hemisphere (20,000deg2) to a depth 4 magnitudes fainterthan 2MASS/DENIS in at least two wavebands J and K.

  3. ��������� ��� ��������������� ��������������…

    https://people.ast.cam.ac.uk/~wyatt/wdgj99.pdf
    19 Apr 2006: 0. 20. 40. Ecl. ipti. c L. atit. ude. 70 80 90 100 110Ecliptic Longitude Relative to Sun. ... 40. -20. 0. 20. 40. 70 80 90 100 110Ecliptic Longitude Relative to Sun.

  4. Dust_in_the_Debris_Disk_Around_HD69830_09Nov2006

    https://people.ast.cam.ac.uk/~wyatt/lbbw07.pdf
    16 Nov 2006: predominantly Mg-rich olivines (80%) and crystalline pyroxenes (20%) (Figure 3). Unlike our. ... Dark blues - crystalline olivines, forsterite and fayalite, in order of 20 µm amplitude.

  5. Estimate of the Number of CPU Nodes to Execute ...

    https://people.ast.cam.ac.uk/~wfcam/ukreview/vircam_cpu_estimate.pdf
    29 Sep 2006: increase the data processing time by approximately 10 to 20%. ... The detailed processing time of this test is:. recipe time = 320 seconds ( 20% for missing functionalities).

  6. mnr_7037.tex

    https://people.ast.cam.ac.uk/~wyatt/gw03.pdf
    19 Apr 2006: and Spangler et al. (2000) are also included here – ISO observed 70per cent of the single A stars but only 20 per cent of single G starswithin 25 pc. ... If the r 3 line in Fig. 2 is extrapolatedfrom 20 to 25 pc, the detections should increase to 20

  7. SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...

    https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf
    19 Apr 2006: areconsistent with a ring of radius 150 20 AU seen at 45 25 inclination. ... would migrate from 150to 0 AU (where it would evaporate) on timescales of 20 Myr(Burns et al.

  8. PDF/48/aa5873-06.pdf.url

    https://people.ast.cam.ac.uk/~wyatt/lwbd06.pdf
    14 Dec 2006: 2004).These two stars are 10–20 Myr old (see Favata et al. ... 1 AU) while (sub)mm surveys probe cold dust (20 K)distant from the star (100’s AU).

  9. https://people.ast.cam.ac.uk/~rgm/wfcsur/meetings/announcement_2.txt

    https://people.ast.cam.ac.uk/~rgm/wfcsur/meetings/announcement_2.txt
    5 Dec 2006: products and archive 14:00 Photometric Calibration (Jones/Hodgkin) 14:20 Astrometric Calibration (Bunclark/Lewis/Irwin) 14:40 Pipeline processing I(including demo) (Lewis/Irwin) 15:20 Tea 15:40 Pipeline

  10. ����������� ��� ������������ ������� �!�"���…

    https://people.ast.cam.ac.uk/~wyatt/wyat05a.pdf
    19 Apr 2006: B-! &-. n u= K G %'. Í 20 10 0 -10 -20RA offset, arcsec. ... $9]! ;9:<8 - P7-& (;! (<$ra A ;{' <9];& C#20% '-&- P (--##; 0B#-3 3;,x,- )/5[?

  11. THE ASTROPHYSICAL JOURNAL, 530 : 329È341, 2000 February 102000. ...

    https://people.ast.cam.ac.uk/~wyatt/tfpk00.pdf
    19 Apr 2006: b) Logarithmic10.8 km levels : 1.3, 1.9, 2.8, 4.2, 6.2, 9.2, 13.7, 20.2, 29.9, 44.3, and 65.5. ... The residual emission (observed minus model ; Fig.4d) at 20 AU from the star is typically 0.2 times that of(0A.3)the lobes.

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